Observational and Dynamical Characterization of Main-belt Comet P/2010 R2 (La Sagra)

We present observations of the recently discovered comet-like main-belt object P/2010 R2 (La Sagra) obtained by Pan-STARRS1 and the Faulkes Telescope-North on Haleakala in Hawaii, the University of Hawaii 2.2 m, Gemini-North, and Keck I telescopes on Mauna Kea, the Danish 1.54 m telescope (operated by the MiNDSTEp consortium) at La Silla, and the Isaac Newton Telescope on La Palma. An antisolar dust tail is observed to be present from 2010 August through 2011 February, while a dust trail aligned with the object's orbit plane is also observed from 2010 December through 2011 August. Assuming typical phase darkening behavior, P/La Sagra is seen to increase in brightness by >1 mag between 2010 August and December, suggesting that dust production is ongoing over this period. These results strongly suggest that the observed activity is cometary in nature (i.e., driven by the sublimation of volatile material), and that P/La Sagra is therefore the most recent main-belt comet to be discovered. We find an approximate absolute magnitude for the nucleus of HR = 17.9 ± 0.2 mag, corresponding to a nucleus radius of ~0.7 km, assuming an albedo of p = 0.05. Comparing the observed scattering surface areas of the dust coma to that of the nucleus when P/La Sagra was active, we find dust-to-nucleus area ratios of Ad /AN = 30-60, comparable to those computed for fellow main-belt comets 238P/Read and P/2008 R1 (Garradd), and one to two orders of magnitude larger than for two other main-belt comets (133P/Elst-Pizarro and 176P/LINEAR). Using optical spectroscopy to search for CN emission, we do not detect any conclusive evidence of sublimation products (i.e., gas emission), finding an upper limit CN production rate of Q CN 100 Myr, suggesting that it is likely native to its current location and that its composition is likely representative of other objects in the same region of the main belt, though the relatively close proximity of the 13:6 mean-motion resonance with Jupiter and the (3,-2,-1) three-body mean-motion resonance with Jupiter and Saturn mean that dynamical instability on larger timescales cannot be ruled out.

The persistent activity of Jupiter-family comets at 3-7 AU

We present an analysis of comet activity based on the Spitzer Space Telescope component of the Survey of the Ensemble Physical Properties of Cometary Nuclei. We show that the survey is well suited to measuring the activity of Jupiter-family comets at 3-7 AU from the Sun. Dust was detected in 33 of 89 targets (37 ± 6%), and we conclude that 21 comets (24 ± 5%) have morphologies that suggest ongoing or recent cometary activity. Our dust detections are sensitivity limited, therefore our measured activity rate is necessarily a lower limit. All comets with small perihelion distances (q <1.8 AU) are inactive in our survey, and the active comets in our sample are strongly biased to post-perihelion epochs. We introduce the quantity ɛfρ, intended to be a thermal emission counterpart to the often reported Afρ, and find that the comets with large perihelion distances likely have greater dust production rates than other comets in our survey at 3-7 AU from the Sun, indicating a bias in the discovered Jupiter-family comet population. By examining the orbital history of our survey sample, we suggest that comets perturbed to smaller perihelion distances in the past 150 yr are more likely to be active, but more study on this effect is needed.

Thermal properties, sizes, and size distribution of Jupiter-family cometary nuclei

We present results from SEPPCoN, an on-going Survey of the Ensemble Physical Properties of Cometary Nuclei. In this report we discuss mid-infrared measurements of the thermal emission from 89 nuclei of Jupiter-family comets (JFCs). All data were obtained in 2006 and 2007 using imaging capabilities of the Spitzer Space Telescope. The comets were typically 4-5 AU from the Sun when observed and most showed only a point-source with little or no extended emission from dust. For those comets showing dust, we used image processing to photometrically extract the nuclei. For all 89 comets, we present new effective radii, and for 57 comets we present beaming parameters. Thus our survey provides the largest compilation of radiometrically-derived physical properties of nuclei to date. We have six main conclusions: (a) The average beaming parameter of the JFC population is 1.03 ± 0.11, consistent with unity; coupled with the large distance of the nuclei from the Sun, this indicates that most nuclei have Tempel 1-like thermal inertia. Only two of the 57 nuclei had outlying values (in a statistical sense) of infrared beaming. (b) The known JFC population is not complete even at 3 km radius, and even for comets that approach to ˜2 AU from the Sun and so ought to be more discoverable. Several recently-discovered comets in our survey have small perihelia and large (above ˜2 km) radii. (c) With our radii, we derive an independent estimate of the JFC nuclear cumulative size distribution (CSD), and we find that it has a power-law slope of around -1.9, with the exact value depending on the bounds in radius. (d) This power-law is close to that derived by others from visible-wavelength observations that assume a fixed geometric albedo, suggesting that there is no strong dependence of geometric albedo with radius. (e) The observed CSD shows a hint of structure with an excess of comets with radii 3-6 km. (f) Our CSD is consistent with the idea that the intrinsic size distribution of the JFC population is not a simple power-law and lacks many sub-kilometer objects.

Outgassing Behavior of C/2012 S1 (ISON) from 2011 September to 2013 June

We report photometric observations for comet C/2012 S1 (ISON) obtained during the time period immediately after discovery (r = 6.28 AU) until it moved into solar conjunction in mid-2013 June using the UH2.2 m, and Gemini North 8 m telescopes on Mauna Kea, the Lowell 1.8 m in Flagstaff, the Calar Alto 1.2 m telescope in Spain, the VYSOS-5 telescopes on Mauna Loa Hawaii and data from the CARA network. Additional pre-discovery data from the Pan STARRS1 survey extends the light curve back to 2011 September 30 (r = 9.4 AU). The images showed a similar tail morphology due to small micron sized particles throughout 2013. Observations at submillimeter wavelengths using the James Clerk Maxwell Telescope on 15 nights between 2013 March 9 (r = 4.52 AU) and June 16 (r = 3.35 AU) were used to search for CO and HCN rotation lines. No gas was detected, with upper limits for CO ranging between 3.5-4.5 × 1027 molecules s-1. Combined with published water production rate estimates we have generated ice sublimation models consistent with the photometric light curve. The inbound light curve is likely controlled by sublimation of CO2. At these distances water is not a strong contributor to the outgassing. We also infer that there was a long slow outburst of activity beginning in late 2011 peaking in mid-2013 January (r ~ 5 AU) at which point the activity decreased again through 2013 June. We suggest that this outburst was driven by CO injecting large water ice grains into the coma. Observations as the comet came out of solar conjunction seem to confirm our models.

Visible-Wavelength Survey of Jupiter-Family Cometary Nuclei as Part of SEPPCoN

We present observations of a statistically-significant number of Jupiter-family cometary nuclei as part of SEPPCoN (Survey of the Ensemble Physical Properties of Cometary Nuclei). We present preliminary results on distributions of albedos and shapes.

Discovery of Main-Belt Comet P/2006 VW139 by Pan-STARRS1

We describe the discovery of comet-like activity in main-belt asteroid (300163) 2006 VW139 (later re-designated as Comet P/2006 VW139) by Pan-STARRS1. We also detail follow-up photometric, spectroscopic, and dynamical analyses of the object.

Caroline: A Search for the Source of Earth's Water

Not Available

Visible-wavelength Observations of Jupiter-family Comet Nuclei as Part of Seppcon.

We present the latest analysis and results from SEPPCoN (Survey of Ensemble Physical Properties of Cometary Nuclei). This on-going survey involves studying 100 JFCs - about 25% of the known population - at both mid-infrared and visible wave-lengths to constrain the distributions of sizes, shapes, spins, and albedos of this population. Having earlier reported results from measuring thermal emissions of our sample nuclei [1,2,3,4], we report here progress on the visible-wavelength observations that we have obtained at many ground-based facilities in Chile, Spain, and the United States. To date we have attempted observations of 91% of our sample of 100 JFCs, and at least 64 of those were successfully detected. In most cases the comets were at heliocentric distances between 3.0 and 6.5 AU so as to decrease the odds of a comet having a coma. Of the 64 detected comets, 48 were apparently bare, having no extended emission. Our datasets are further augmented by archival data and photometry from the NEAT program [5]. An important goal of SEPPCoN is to accumulate a large comprehensive set of high quality physical data on cometary nuclei in order to make accurate statistical comparisons with other minor-body populations such as Trojans, Centaurs, and Kuiper-belt objects. Information on the size, shape, spin-rate, albedo and color distributions is critical for understanding their origins and evolutionary processes affecting them.

Spitzer observations of the asteroid-comet transition object and potential spacecraft target 107P (4015) Wilson-Harrington

Context: Near-Earth asteroid-comet transition object 107P/ (4015) Wilson-Harrington is a possible target of the joint European Space Agency (ESA) and Japanese Aerospace Exploration Agency (JAXA) Marco Polo sample return mission. Physical studies of this object are relevant to this mission, and also to understanding its asteroidal or cometary nature. Aims: Our aim is to obtain significant new constraints on the surface thermal properties of this object. Methods: We present mid-infrared photometry in two filters (16 and 22 μm) obtained with NASA's Spitzer Space Telescope on February 12, 2007, and results from the application of the Near Earth Asteroid Thermal Model (NEATM). We obtained high S/N in two mid-IR bands allowing accurate measurements of its thermal emission. Results: We obtain a well constrained beaming parameter (η = 1.39±0.26) and obtain a diameter and geometric albedo of D = 3.46±0.32 km, and pV = 0.059±0.011. We also obtain similar results when we apply this best-fitting thermal model to single-band mid-IR photometry reported by Campins et al. (1995, P&SS, 43, 733), Kraemer et al. (2005, AJ, 130, 2363) and Reach et al. (2007, Icarus, 191, 298). Conclusions: The albedo of 4015 Wilson-Harrington is low, consistent with those of comet nuclei and primitive C-, P-, D-type asteorids. We establish a rough lower limit for the thermal inertia of W-H of 60 Jm-2s-0.5 K-1 when it is at r = 1 AU, which is slightly over the limit of 30 Jm-2 s-0.5 K-1 derived by Groussin et al. (2009, Icarus, 199, 568) for the thermal inertia of the nucleus of comet 22P/Kopff.

A Hundred Comets: The Visual-Wavelength Observations of the Survey of Ensemble Physical Properties of Cometary Nuclei (SEPPCoN)

We present new results from SEPPCoN, a Survey of Ensemble Physical Properties of Cometary Nuclei. This project is currently surveying 100 Jupiter-family comets (JFCs) to measure the mid-infrared thermal emission and visible reflected sunlight of the nuclei. The scientific goal is to determine the distributions of radius, geometric albedo, thermal inertia, axial ratio, and color among the JFC nuclei. In the past we have presented results from the completed mid-IR observations of our sample [1]; here we present preliminary results from ongoing, broadband visible-wavelength observations of nuclei obtained from a variety of ground-based facilities (Mauna Kea, Cerro Pachon, La Silla, La Palma, Apache Point, Table Mtn., and Palomar Mtn.), including contributions from the Near Earth Asteroid Telescope project (NEAT) archive. The nuclei were observed at high heliocentric distance (usually over 4 AU) and so many comets show either no or little contamination from dust coma. While several nuclei have been observed as snapshots, we have multiepoch photometry for many of our targets. With our datasets we are building a large database of photometry, and such a database is essential to the derivation of albedo and shape of a large number of nuclei, and to the understanding of biases in the survey. Support for this work was provided by NSF and the NASA Planetary Astronomy program. Reference: [1] Fernandez, Y.R., et al. 2007, BAAS 39, 827.

Comet C/2012 S1 (ISON): Observations of the Dust Grains from SOFIA and of the Atomic Gas from NSO Dunn and McMath-Pierce Solar Telescopes (Invited)

Comet C/2012 S1 (ISON) is unique in that it is a dynamically new comet derived from the Oort cloud reservoir of comets with a sun-grazing orbit. Infrared (IR) and visible wavelength observing campaigns were planned on NASA's Stratospheric Observatory For Infrared Astronomy (SOFIA) and on National Solar Observatory Dunn (DST) and McMath-Pierce Solar Telescopes, respectively. We highlight our early results. SOFIA (+FORCAST [1]) mid- to far-IR images and spectroscopy (~5-35 μm) of the dust in the coma of ISON are to be obtained by the ISON-SOFIA Team during a flight window 2013 Oct 21-23 UT (r_h≈1.18 AU). Dust characteristics, identified through the 10 μm silicate emission feature and its strength [2], as well as spectral features from cometary crystalline silicates (Forsterite) at 11.05-11.2 μm, and near 16, 19, 23.5, 27.5, and 33 μm are compared with other Oort cloud comets that span the range of small and/or highly porous grains (e.g., C/1995 O1 (Hale-Bopp) [3,4,5] and C/2001 Q4 (NEAT) [6]) to large and/or compact grains (e.g., C/2007 N4 (Lulin) [7] and C/2006 P1 (McNaught) [8]). Measurement of the crystalline peaks in contrast to the broad 10 and 20 μm amorphous silicate features yields the cometary silicate crystalline mass fraction [9], which is a benchmark for radial transport in our protoplanetary disk [10]. The central wavelength positions, relative intensities, and feature asymmetries for the crystalline peaks may constrain the shapes of the crystals [11]. Only SOFIA can look for cometary organics in the 5-8 μm region. Spatially resolved measurements of atoms and simple molecules from when comet ISON is near the Sun (r_h<0.4 AU, near Nov-20--Dec-03 UT) were proposed for by the ISON-DST Team. Comet ISON is the first comet since comet Ikeya-Seki (1965f) [12,13] suitable for studying the alkalai metals Na and K and the atoms specifically attributed to dust grains including Mg, Si, Fe, as well as Ca. DST's Horizontal Grating Spectrometer (HGS) measures 4 settings: Na I, K, C2 to sample cometary organics (along with Mg I), and [O I] as a proxy for activity from water [14] (along with Si I and Fe I). State-of-the-art instruments that will also be employed include IBIS [15], which is a Fabry-Perot spectral imaging system that concurrently measures lines of Na, K, Ca II, or Fe, and ROSA (CSUN/QUB) [16], which is a rapid imager that simultaneously monitors Ca II or CN. From McMath-Pierce, the Solar-Stellar Spectrograph also will target ISON (320-900 nm, R~21,000, r_h

Regularization and Bang-bang conjugate times in optimal control

Consideramos o problema de controlo óptimo de tempo mínimo para sistemas de controlo mono-entrada e controlo afim num espaço de dimensão finita com condições inicial e final fixas, onde o controlo escalar toma valores num intervalo fechado. Quando aplicamos o método de tiro a este problema, vários obstáculos podem surgir uma vez que a função de tiro não é diferenciável quando o controlo é bang-bang. No caso bang-bang os tempos conjugados são teoricamente bem definidos para este tipo de sistemas de controlo, contudo os algoritmos computacionais directos disponíveis são de difícil aplicação. Por outro lado, no caso suave o conceito teórico e prático de tempos conjugados é bem conhecido, e ferramentas computacionais eficazes estão disponíveis. Propomos um procedimento de regularização para o qual as soluções do problema de tempo mínimo correspondente dependem de um parâmetro real positivo suficientemente pequeno e são definidas por funções suaves em relação à variável tempo, facilitando a aplicação do método de tiro simples. Provamos, sob hipóteses convenientes, a convergência forte das soluções do problema regularizado para a solução do problema inicial, quando o parâmetro real tende para zero. A determinação de tempos conjugados das trajectórias localmente óptimas do problema regularizado enquadra-se na teoria suave conhecida. Provamos, sob hipóteses adequadas, a convergência do primeiro tempo conjugado do problema regularizado para o primeiro tempo conjugado do problema inicial bang-bang, quando o parâmetro real tende para zero. Consequentemente, obtemos um algoritmo eficiente para a computação de tempos conjugados no caso bang-bang.

Role of intracellular signaling pathways activated in fibroblasts in response to lipoproteins

Summary The best described physiological function of low-density lipoproteins (LDL) is to transport cholesterol to target tissues. LDL deliver their cholesterol cargo to cells following their interaction with the LDL receptor. LDL, when their vascular concentrations increase, have also been implicated in pathologies such as atherosclerosis. Among the cell types that are found in blood vessels, endothelial and smooth muscle cells have dominated cellular research on atherosclerotic mechanisms and LDL activation of signaling pathways, while very little is known about adventitial fibroblast activation caused by elevated lipoprotein levels. Since fibroblasts participate in wound repair and since it has recently been recognized that fibroblasts may play pivotal roles in vascular remodeling and repair of injury, we assessed whether lipoproteins affect fibroblast function. We have found that LDL specifically mediate the activation of a class of mitogen-activated protein kinases (MAPKs): the p38 MAPKs. The activation of this pathway in turn modulates cell shape by promoting lamellipodia formation and extensive cell spreading. This is of particular interest because it provides a mechanism by which LDL can promote wound healing or vessel wall remodeling as observed during the development of atherosclerosis. In order to understand the molecular mechanisms by which LDL induce p38 activation we searched for the component in the LDL particle responsible for the induction of this pathway. We found that cholesterol is the major component of lipoprotein particles that mediates their ability to stimulate the p38 MAPK pathway. Furthermore, we investigated the cellular mechanisms underlying the ability of LDL to induce cell shape changes and whether this could participate in wound repair. Our recent data demonstrates that the capacity of LDL to induce fibroblast spreading relies on their ability to stimulate IL-8 secretion, which in turn leads to accelerated wound healing. LDL-induced IL-8 production and subsequent wound closure are impaired upon inhibition of the p38 MAPK pathway indicating that the LDL-induced spreading and accelerated wound sealing rely on the ability of LDL to stimulate IL-8 secretion in a p38 MAPK-dependent manner. Therefore, regulation of fibroblast shape and migration by lipoproteins may be relevant to atherosclerosis that is characterized by increased LDL-cholesterol levels, IL-8 production and extensive remodeling of the vessel wall. Résumé: La fonction physiologique des lipoprotéines à faible densité (LDL) la mieux décrite est celle du transport du cholestérol aux tissus cibles. Les LDL livrent leur cargaison de cholestérol aux cellules après leur interaction avec le récepteur au LDL. Une concentration vasculaire des LDL augmenté est également impliquée dans le développement de l'athérosclérose. Parmi les types de cellule présents dans les vaisseaux sanguins, les cellules endothéliales et les cellules du muscle lisse ont dominé la recherche cellulaire sur les mécanismes athérosclérotiques et sur l'activation par les LDL des voies de signalisation intracellulaire. A l'inverse peu de choses sont connues sur l'activation des fibroblastes de l'adventice par les lipoprotéines. Puisqu'il a été récemment reconnu que les fibroblastes peuvent jouer un rôle central dans la remodélisation vasculaire et la réparation tissulaire, nous avons étudié si les lipoprotéines affectent la fonction des fibroblastes. Nous avons constaté que les LDL activent spécifiquement une classe de protéines kinases: les p38 MAPK (mitogen-activated protein kinases). L'activation de cette voie module à son tour la forme de la cellule en favorisant la formation de lamellipodes et l'agrandissement des cellules. Cela a un intérêt particulier car il fournit un mécanisme par lequel les LDL peuvent promouvoir la cicatrisation ou la remodélisation des parois vasculaires comme observés lors du développement de l'athérosclérose. Pour comprendre les mécanismes moléculaires par lesquels les LDL provoquent l'activation des p38 MAPK, nous avons cherché à identifier les composants dans la particule de LDL responsables de l'induction de cette voie. Nous avons constaté que le cholestérol est l'élément principal des particules de lipoprotéine qui contrôle leur capacité à stimuler la voie des p38 MAPK. En outre, nous avons examiné les mécanismes cellulaires responsables de la capacité des LDL à induire des changements dans la forme des cellules. Nos données récentes démontrent que la capacité des LDL à induire l'agrandissement des cellules, ainsi que leur aptitude à favoriser la cicatrisation, reposant sur leur capacité à stimuler la sécrétiond'IL-8. La production d'IL-8 induite par les LDL est bloquée par l'inhibition de la voie p38 MAPK, ce qui indique que l'étalement des cellules induit par les LDL ainsi que l'accélération de la cicatrisation sont liés à la capacité des LDL à stimuler la sécrétion d'IL8 via l'activation des p38 MAPK. La régulation de la forme et de la migration des fibroblastes par les lipoprotéines peuvent donc participer au développement de l'athérosclérose qui est caractérisée par l'augmentation des niveaux de production de LDL-cholestérol et d'IL-8 ainsi que par une remodélisation augmentée de la paroi du vaisseau.

Etude des propriétés dynamiques de la sécrétion régulée des vésicules glutamatergiques des astrocytes

RESUME GRAND PUBLICLe cerveau est composé de différents types cellulaires, dont les neurones et les astrocytes. Faute de moyens pour les observer, les astrocytes sont très longtemps restés dans l'ombre alors que les neurones, bénéficiant des outils ad hoc pour être stimulés et étudiés, ont fait l'objet de toutes les attentions. Le développement de l'imagerie cellulaire et des outils fluorescents ont permis d'observer ces cellules non électriquement excitables et d'obtenir des informations qui laissent penser que ces cellules sont loin d'être passives et participent activement au fonctionnement cérébral. Cette participation au fonctionnement cérébral se fait en partie par le biais de la libération de substances neuro-actives (appellées gliotransmetteurs) que les astrocytes libèrent à proximité des synapses permettant ainsi de moduler le fonctionnement neuronal. Cette libération de gliotransmetteurs est principalement causée par l'activité neuronale que les astrocytes sont capables de sentir. Néanmoins, nous savons encore peu de chose sur les propriétés précises de la libération des gliotransmetteurs. Comprendre les propriétés spatio-temporelles de cette libération est essentiel pour comprendre le mode de communication de ces cellules et leur implication dans la transmission de l'information cérébrale. En utilisant des outils fluorescents récemment développés et en combinant différentes techniques d'imagerie cellulaire, nous avons pu obtenir des informations très précises sur la libération de ces gliotransmetteurs par les astrocytes. Nous avons ainsi confirmé que cette libération était un processus très rapide et qu'elle était contrôlée par des augmentations de calcium locales et rapides. Nous avons également décrit une organisation complexe de la machinerie supportant la libération des gliotransmetteurs. Cette organisation complexe semble être à la base de la libération extrêmement rapide des gliotransmetteurs. Cette rapidité de libération et cette complexité structurelle semblent indiquer que les astrocytes sont des cellules particulièrement adaptées à une communication rapide et qu'elles peuvent, au même titre que les neurones dont elles seraient les partenaires légitimes, participer à la transmission et à l'intégration de l'information cérébrale.RESUMEDe petites vésicules, les « SLMVs » ou « Synaptic Like MicroVesicles », exprimant des transporteurs vésiculaires du glutamate (VGluTs) et libérant du glutamate par exocytose régulée, ont récemment été décrites dans les astrocytes en culture et in situ. Néanmoins, nous savons peu de chose sur les propriétés précises de la sécrétion de ces SLMVs. Contrairement aux neurones, le couplage stimulussécrétion des astrocytes n'est pas basé sur l'ouverture des canaux calciques membranaires mais nécessite l'intervention de seconds messagers et la libération du calcium par le reticulum endoplasmique (RE). Comprendre les propriétés spatio-temporelles de la sécrétion astrocytaire est essentiel pour comprendre le mode de communication de ces cellules et leur implication dans la transmission de l'information cérébrale. Nous avons utilisé des outils fluorescents récemment développés pour étudier le recyclage des vésicules synaptiques glutamatergiques comme les colorants styryles et la pHluorin afin de pouvoir suivre la sécrétion des SLMVs à l'échelle de la cellule mais également à l'échelle des évènements. L'utilisation combinée de l'épifluorescence et de la fluorescence à onde évanescente nous a permis d'obtenir une résolution temporelle et spatiale sans précédent. Ainsi avons-nous confirmé que la sécrétion régulée des astrocytes était un processus très rapide (de l'ordre de quelques centaines de millisecondes). Nous avons découvert que cette sécrétion est contrôlée par des augmentations de calcium locales et rapides. Nous avons également décrit des compartiments cytosoliques délimités par le RE à proximité de la membrane plasmique et contenant les SLMVs. Cette organisation semble être à la base du couplage rapide entre l'activation des GPCRs et la sécrétion. L'existence de compartiments subcellulaires indépendants permettant de contenir les messagers intracellulaires et de limiter leur diffusion semble compenser de manière efficace la nonexcitabilité électrique des astrocytes. Par ailleurs, l'existence des différents pools de vésicules recrutés séquentiellement et fusionnant selon des modalités distinctes ainsi que l'existence de mécanismes permettant le renouvellement de ces pools lors de la stimulation suggèrent que les astrocytes peuvent faire face à une stimulation soutenue de leur sécrétion. Ces données suggèrent que la libération de gliotransmetteurs par exocytose régulée n'est pas seulement une propriété des astrocytes en culture mais bien le résultat d'une forte spécialisation de ces cellules pour la sécrétion. La rapidité de cette sécrétion donne aux astrocytes toutes les compétences pour pouvoir intervenir de manière active dans la transmission et l'intégration de l'information.ABSTRACTRecently, astrocytic synaptic like microvesicles (SLMVs), that express vesicular glutamate transporters (VGluTs) and are able to release glutamate by Ca2+-dependent regulated exocytosis, have been described both in tissue and in cultured astrocytes. Nevertheless, little is known about the specific properties of regulated secretion in astrocytes. Important differences may exist between astrocytic and neuronal exocytosis, starting from the fact that stimulus-secretion coupling in astrocytes is voltage independent, mediated by G-protein-coupled receptors and the release of Ca2+ from internal stores. Elucidating the spatiotemporal properties of astrocytic exo-endocytosis is, therefore, of primary importance for understanding the mode of communication of these cells and their role in brain signaling. We took advantage of fluorescent tools recently developed for studying recycling of glutamatergic vesicles at synapses like styryl dyes and pHluorin in order to follow exocytosis and endocytosis of SLMVs at the level of the entire cell or at the level of single event. We combined epifluorescence and total internal reflection fluorescence imaging to investigate, with unprecedented temporal and spatial resolution, the events underlying the stimulus-secretion in astrocytes. We confirmed that exo-endocytosis process in astrocytes proceeds with a time course on the millisecond time scale. We discovered that SLMVs exocytosis is controlled by local and fast Ca2+ elevations; indeed submicrometer cytosolic compartments delimited by endoplasmic reticulum (ER) tubuli reaching beneath the plasma membrane and containing SLMVs. Such complex organization seems to support the fast stimulus-secretion coupling reported here. Independent subcellular compartments formed by ER, SLMVs and plasma membrane containing intracellular messengers and limiting their diffusion seem to compensate efficiently the non-electrical excitability of astrocytes. Moreover, the existence of two pools of SLMVs which are sequentially recruited suggests a compensatory mechanisms allowing the refill of SLMVs and supporting exocytosis process over a wide range of multiple stimuli. These data suggest that regulated secretion is not only a feature of cultured astrocytes but results from a strong specialization of these cells. The rapidity of secretion demonstrates that astrocytes are able to actively participate in brain information transmission and processing.

Effet de l'atorvastatine et de l'amlodipine sur le remodelage vasculaire dans l'hypertension

Résumé Introduction L’amlodipine et l’atorvastatine offrent des avantages thérapeutiques au-delà de leur indication primaire, soit la réduction de la pression artérielle et des lipides sanguins, respectivement. L’amlodipine induit l’apoptose des cellules de muscle lisse vasculaire (CMLV) in vivo, contribuant à la régression de l'hypertrophie aortique chez le rat spontanément hypertendu (SHR). L'atorvastatine induit l’apoptose des CMLV in vitro, un effet proportionnel à la dose. Toutefois, cet effet reste à être démontré in vivo. Nous postulons que l’atorvastatine induira la régression de l’hypertrophie aortique via l’apoptose des CMLV chez le SHR, et que la combinaison de l’amlodipine et de l’atorvastatine aura un effet synergique sur la régression de l’hypertrophie aortique via l’apoptose des CMLV chez le SHR. Méthodologie L’amlodipine et l’atorvastatine ont été administrées à des SHR âgés de 11 semaines durant trois ou six semaines, individuellement ou en combinaison. Les points principaux à l'étude étaient le remodelage vasculaire et la pression artérielle. La fragmentation et le contenu en ADN, le stress oxydant, le taux de cholestérol et les niveaux de nitrates ont aussi été mesurés. Résultats Lorsque l’atorvastatine a été administrée seule, une diminution significative du stress oxydant et de la pression artérielle a été observée après trois et six semaines de traitement, respectivement. Par contre, aucune différence n’a pu être décelée quant au remodelage vasculaire. L'amlodipine a réduit la pression artérielle et l'hypertrophie aortique de façon dépendante de la dose. Une diminution significative de l'hyperplasie a été détectée après trois semaines de traitement avec la combinaison, et après six semaines avec une faible dose d'amlodipine. Conclusion Nos résultats ne supportent pas l'hypothèse que l'atorvastatine induit l'apoptose des CMLV in vivo. Par contre, lorsque combinée à l'amlodipine, elle pourrait ajouter un bénéfice supplémentaire au niveau de la réduction de l'hyperplasie aortique.