Astrophysical parameters and orbital solution of the peculiar X-ray transient IGR J00370+6122

Context. BD + 60° 73 is the optical counterpart of the X-ray source IGR J00370+6122, a probable accretion-powered X-ray pulsar. The X-ray light curve of this binary system shows clear periodicity at 15.7 d, which has been interpreted as repeated outbursts around the periastron of an eccentric orbit. Aims. We aim to characterise the binary system IGR J00370+6122 by deriving its orbital and physical parameters. Methods. We obtained high-resolution spectra of BD + 60° 73 at different epochs. We used the fastwind code to generate a stellar atmosphere model to fit the observed spectrum and obtain physical magnitudes. The synthetic spectrum was used as a template for cross-correlation with the observed spectra to measure radial velocities. The radial velocity curve provided an orbital solution for the system. We also analysed the RXTE/ASM and Swift/BAT light curves to confirm the stability of the periodicity. Results. BD + 60° 73 is a BN0.7 Ib low-luminosity supergiant located at a distance ~3.1 kpc, in the Cas OB4 association. We derive Teff = 24 000 K and log gc = 3.0, and chemical abundances consistent with a moderately high level of evolution. The spectroscopic and evolutionary masses are consistent at the 1-σ level with a mass M∗ ≈ 15 M⊙. The recurrence time of the X-ray flares is the orbital period of the system. The neutron star is in a high-eccentricity (e = 0.56 ± 0.07) orbit, and the X-ray emission is strongly peaked around orbital phase φ = 0.2, though the observations are consistent with some level of X-ray activity happening at all orbital phases. Conclusions. The X-ray behaviour of IGR J00370+6122 is reminiscent of “intermediate” supergiant X-ray transients, though its peak luminosity is rather low. The orbit is somewhat wider than those of classical persistent supergiant X-ray binaries, which when combined with the low luminosity of the mass donor, explains the low X-ray luminosity. IGR J00370+6122 will very likely evolve towards a persistent supergiant system, highlighting the evolutionary connection between different classes of wind-accreting X-ray sources.

Measuring the stellar wind parameters in IGR J17544-2619 and Vela X-1 constrains the accretion physics in supergiant fast X-ray transient and classical supergiant X-ray binaries

Context. Classical supergiant X-ray binaries (SGXBs) and supergiant fast X-ray transients (SFXTs) are two types of high-mass X-ray binaries (HMXBs) that present similar donors but, at the same time, show very different behavior in the X-rays. The reason for this dichotomy of wind-fed HMXBs is still a matter of debate. Among the several explanations that have been proposed, some of them invoke specific stellar wind properties of the donor stars. Only dedicated empiric analysis of the donors’ stellar wind can provide the required information to accomplish an adequate test of these theories. However, such analyses are scarce. Aims. To close this gap, we perform a comparative analysis of the optical companion in two important systems: IGR J17544-2619 (SFXT) and Vela X-1 (SGXB). We analyze the spectra of each star in detail and derive their stellar and wind properties. As a next step, we compare the wind parameters, giving us an excellent chance of recognizing key differences between donor winds in SFXTs and SGXBs. Methods. We use archival infrared, optical and ultraviolet observations, and analyze them with the non-local thermodynamic equilibrium (NLTE) Potsdam Wolf-Rayet model atmosphere code. We derive the physical properties of the stars and their stellar winds, accounting for the influence of X-rays on the stellar winds. Results. We find that the stellar parameters derived from the analysis generally agree well with the spectral types of the two donors: O9I (IGR J17544-2619) and B0.5Iae (Vela X-1). The distance to the sources have been revised and also agree well with the estimations already available in the literature. In IGR J17544-2619 we are able to narrow the uncertainty to d = 3.0 ± 0.2 kpc. From the stellar radius of the donor and its X-ray behavior, the eccentricity of IGR J17544-2619 is constrained to e< 0.25. The derived chemical abundances point to certain mixing during the lifetime of the donors. An important difference between the stellar winds of the two stars is their terminal velocities (ν∞ = 1500 km s-1 in IGR J17544-2619 and ν∞ = 700 km s-1 in Vela X-1), which have important consequences on the X-ray luminosity of these sources. Conclusions. The donors of IGR J17544-2619 and Vela X-1 have similar spectral types as well as similar parameters that physically characterize them and their spectra. In addition, the orbital parameters of the systems are similar too, with a nearly circular orbit and short orbital period. However, they show moderate differences in their stellar wind velocity and the spin period of their neutron star which has a strong impact on the X-ray luminosity of the sources. This specific combination of wind speed and pulsar spin favors an accretion regime with a persistently high luminosity in Vela X-1, while it favors an inhibiting accretion mechanism in IGR J17544-2619. Our study demonstrates that the relative wind velocity is critical in class determination for the HMXBs hosting a supergiant donor, given that it may shift the accretion mechanism from direct accretion to propeller regimes when combined with other parameters.

Blood markers and recurrence of stroke in patients with transient ischemic attack

Trabalho Final do Curso de Mestrado Integrado em Medicina, Faculdade de Medicina, Universidade de Lisboa, 2014

Implications physiopathologiques de la Nestine lors du remodelage pulmonaire et cardiaque à la suite de l’infarctus du myocarde, du diabète et de l’hypertension pulmonaire

Il est reconnu que la protéine filamenteuse intermédiaire Nestine est exprimée lors du processus de cicatrisation et du remodelage fibrotique. De plus, nous avons identifié l’expression de la Nestine au sein de deux populations distinctes qui sont directement impliquées dans les réponses de fibroses réparative et réactive. Ainsi, une population de cellules souches neurales progénitrices résidentes du coeur de rat adulte exprime la Nestine et a été identifiée à titre de substrat de l’angiogenèse et de la neurogenèse cardiaque. Également, la Nestine est exprimée par les myofibroblastes cicatriciels cardiaques et il a été établi que la protéine filamenteuse intermédiaire joue un rôle dans la prolifération de ces cellules. Ainsi, l’objectif général de cette thèse était de mieux comprendre les évènements cellulaires impliqués dans la réponse neurogénique des cellules souches neurales progénitrices résidentes cardiaques Nestine(+) (CSNPRCN(+)) lors de la fibrose réparative cardiaque et d’explorer si l’apparition de fibroblastes Nestine(+) est associée avec la réponse de fibrose réactive secondaire du remodelage pulmonaire. Une première publication nous a permis d’établir qu’il existe une régulation à la hausse de l’expression de la GAP43 (growth associated protein 43) et que cet événement transitoire précède l’acquisition d’un phénotype neuronal par les CSNPRCN(+) lors du processus de cicatrisation cardiaque chez le rat ayant subi un infarctus du myocarde. De plus, la surimposition de la condition diabétique de type 1, via l’injection unique de Streptozotocine chez le rat, abolit la réponse neurogénique des CSNPRCN(+), qui est normalement induite à la suite de l’ischémie cardiaque ou de l’administration de 6-hydroxydopamine. Le second article a démontré que le développement aigu de la fibrose pulmonaire secondaire de l’infarctus du myocarde chez le rat est associé avec une augmentation de l’expression protéique de la Nestine et de l’apparition de myofibroblastes pulmonaires Nestine(+). Également, le traitement de fibroblastes pulmonaires avec des facteurs de croissances peptidiques pro-fibrotiques a augmenté l’expression de la Nestine par ces cellules. Enfin, le développement initial de la condition diabétique de type 1 chez le rat est associé avec une absence de fibrose réactive pulmonaire et à une réduction significative des niveaux protéiques et d’ARN messager de la Nestine pulmonaire. Finalement, la troisième étude représentait quant à elle un prolongement de la deuxième étude et a alors examiné le remodelage pulmonaire chronique chez un modèle établi d’hypertension pulmonaire. Ainsi, les poumons de rats adultes mâles soumis à l’hypoxie hypobarique durant 3 semaines présentent un remodelage vasculaire, une fibrose réactive et une augmentation des niveaux d’ARN messager et de la protéine Nestine. De plus, nos résultats ont démontré que la Nestine, plutôt que l’alpha-actine du muscle lisse, est un marqueur plus approprié des diverses populations de fibroblastes pulmonaires activés. Également, nos données suggèrent que les fibroblastes pulmonaires activés proviendraient en partie de fibroblastes résidents, ainsi que des processus de transition épithélio-mésenchymateuse et de transition endothélio-mésenchymateuse. Collectivement, ces études ont démontré que des populations distinctes de cellules Nestine(+) jouent un rôle majeur dans la fibrose réparative cardiaque et la fibrose réactive pulmonaire.

Transient Activation of Meox1 Is an Early Component of the Gene Regulatory Network Downstream of Hoxa2

Hox genes encode transcription factors that regulate morphogenesis in all animals with bilateral symmetry. Although Hox genes have been extensively studied, their molecular function is not clear in vertebrates, and only a limited number of genes regulated by Hox transcription factors have been identified. Hoxa2 is required for correct development of the second branchial arch, its major domain of expression. We now show that Meox1 is genetically downstream from Hoxa2 and is a direct target. Meox1 expression is downregulated in the second arch of Hoxa2 mouse mutant embryos. In chromatin immunoprecipitation (ChIP), Hoxa2 binds to the Meox1 proximal promoter. Two highly conserved binding sites contained in this sequence are required for Hoxa2-dependent activation of the Meox1 promoter. Remarkably, in the absence of Meox1 and its close homolog Meox2, the second branchial arch develops abnormally and two of the three skeletal elements patterned by Hoxa2 are malformed. Finally, we show that Meox1 can specifically bind the DNA sequences recognized by Hoxa2 on its functional target genes. These results provide new insight into the Hoxa2 regulatory network that controls branchial arch identity.

Microglial Cells Prevent Hemorrhage in Neonatal Focal Arterial Stroke

Perinatal stroke leads to significant morbidity and long-term neurological and cognitive deficits. The pathophysiological mechanisms of brain damage depend on brain maturation at the time of stroke. To understand whether microglial cells limit injury after neonatal stroke by preserving neurovascular integrity, we subjected postnatal day 7 (P7) rats depleted of microglial cells, rats with inhibited microglial TGFbr2/ALK5 signaling, and corresponding controls, to transient middle cerebral artery occlusion (tMCAO). Microglial depletion by intracerebral injection of liposome-encapsulated clodronate at P5 significantly reduced vessel coverage and triggered hemorrhages in injured regions 24 h after tMCAO. Lack of microglia did not alter expression or intracellular redistribution of several tight junction proteins, did not affect degradation of collagen IV induced by the tMCAO, but altered cell types producing TGFβ1 and the phosphorylation and intracellular distribution of SMAD2/3. Selective inhibition of TGFbr2/ALK5 signaling in microglia via intracerebral liposome-encapsulated SB-431542 delivery triggered hemorrhages after tMCAO, demonstrating that TGFβ1/TGFbr2/ALK5 signaling in microglia protects from hemorrhages. Consistent with observations in neonatal rats, depletion of microglia before tMCAO in P9 Cx3cr1(GFP/+)/Ccr2(RFP/+) mice exacerbated injury and induced hemorrhages at 24 h. The effects were independent of infiltration of Ccr2(RFP/+) monocytes into injured regions. Cumulatively, in two species, we show that microglial cells protect neonatal brain from hemorrhage after acute ischemic stroke. SIGNIFICANCE STATEMENT The pathophysiological mechanisms of brain damage depend on brain maturation at the time of stroke. We assessed whether microglial cells preserve neurovascular integrity after neonatal stroke. In neonatal rats, microglial depletion or pharmacological inhibition of TGFbr2/ALK5 signaling in microglia triggered hemorrhages in injured regions. The effect was not associated with additional changes in expression or intracellular redistribution of several tight junction proteins or collagen IV degradation induced by stroke. Consistent with observations in neonatal rats, microglial depletion in neonatal mice exacerbated stroke injury and induced hemorrhages. The effects were independent of infiltration of monocytes into injured regions. Thus, microglia protect neonatal brain from ischemia-induced hemorrhages, and this effect is consistent across two species.

Rolling resistance of tires measured under transient and equilibrium conditions on Calspan's tire research. Final report.

Transportation Department, Office of the Assistant Secretary for Systems Development and Technology, Washington, D.C.

Equilibrium and transient rolling resistance of truck tires measured on Calspan's tire research facility. Final report.

Transportation Department, Office of Noise Abatement, Washington, D.C.

CRASH: a computer simulator of non-linear transient response of structures, basis for car crash simulation. Research report.

National Highway Traffic Safety Administration, Washington, D.C.

Rolling resistance of truck tires as measured under equilibrium and transient conditions on Calspan's tire research facility. Final report.

Transportation Department, Office of Noise Abatement, Washington, D.C.

Transient viscous flow around an elliptic cylinder /

Originally presented as the author's thesis (M.S.), University of Illinois at Urbana-Champaign.

Transient surface temperature measurements.

Mode of access: Internet.

Interim report on transient heat-transfer measurements of catalytic recombination in a step-function flow of atomic oxygen.

"AFOSR 3203. Contract no. AF 49(638)-782."