Angular momentum of S0 galaxies

The aim of this thesis is to study the angular momentum of a sample of S0 galaxies. In the quest to understand whether the formation of S0 galaxies is more closely linked to that of ellipticals or that of spirals, our goal is to compare the amount of their specific angular momentum as a function of stellar mass with respect to spirals. Through kinematic comparison between these different classes of galaxies we aim to understand if a scenario of passive evolution, in which the galaxy’s gas is consumed and the star formation is quenched, can be considered as plausible mechanism to explain the transformation from spirals to S0s. In order to derive the structural and photometric parameters of galaxy sub-components we performed a bulge-disc decomposition of optical images using GALFIT. The stellar kinematic of the galaxies was measured using integral field spectroscopic data from CALIFA survey. The development of new original software, based on a Monte Carlo Markov Chain algorithm, allowed us to obtain the values of the line of sight velocity and velocity dispersion of disc and bulge components. The result that we obtained is that S0 discs have a distribution of stellar specific angular momentum that is in full agreement with that of spiral discs, so the mechanism of simple fading can be considered as one of the most important for transformation from spirals to S0s.

Towards Night

Sixty artists explore the nocturnal. Curated by Tom Hammick. The evening hour too gives us the irresponsibility which darkness and lamplight bestow. We are no longer quite ourselves. – Virginia Woolf, Street Haunting: A London Adventure, 1930 Towards Night is an exhibition exploring the nocturnal through paintings, prints and drawings by over sixty artists. Drawing on the nineteenth century European Romantic tradition, the show surveys contemporary and historical connections to wonderment and dystopia at dusk, twilight, night and dawn. Towards Night juxtaposes key paintings and prints by Constable, Friedrich, Munch, Nolde, Palmer and Turner, some of the best known visionaries of the Romantic tradition with contemporary artists who work with the transformative aspects of nightfall to convey emotional responses of awe, anxiety and solitude, love and loss, revelry, insomnia, and journey’s end. The exhibition opens with direct and positive responses to the natural world; Marc Chagall’s exotic dreamlike evening in The Poet Reclining (1915) sits close to eighteenth century Indian miniatures depicting brightly painted figures offset against darkening monsoon clouds, and William Crozier’s Balcony at Night, Antibes (2007), of a plant, blue and iridescent against the cool night sky. As the exhibition progresses, the dystopias become darker and more disturbing, and the connections between artists and works intensify: Emma Stibbon’s Rome Aqueduct (2011) takes on a heightened sense of pathos alongside Caspar David Friedrich’s Winter Landscape (1811); Peter Doig’s cinematic Echo Lake (1998) conjures up an increased sense of contemporary angst; and Prunella Clough’s False Flower (1993), a magical tree defying brutalism by growing out of concrete, becomes more miraculous near Night Shift (2015) Nick Carrick’s tomblike high rise. Tom Hammick’s Violetta Alone (2015) and Michael Craig Martin’s Ash Tray (2015), reinforce hedonistic aspects of night-time revelry alongside Four AM, Betsy Dadd’s young woman drinking in the early hours of the morning and L.S. Lowry’s drunken people in a pub in The Crowd (1922). In the final room, a cluster of works explores dreams and insomnia, from Louise Bourgeois’ Spirals (2010) to Munch’s lovers embracing in The Kiss (1902). Tom Hammick, curator of the show said “This exhibition has grown way beyond its original conception, to become a magnificent survey of painting and printmaking from over two hundred years based around the central tenet of night. The exhibition is a kind of painterly response to the way figurative artists use their artistic heroes as starting points for their own work, both compositionally and emotionally.” Artists featured in Towards Night: Christiane Baumgarter, Michael Craig-Martin, Julian Opie, Will Gill, Merlin James, Howard Hodgkin, WillIam Scott, Patrick Caulfield, George Shaw, Stephen Chambers, Basil Beattie, Betsy Dadd, Christopher Le Brun, L.S Lowry, Andrew Cranston, David Willetts, James Fisher, Emma Stibbon, Vija Celmins, William Blake, William Crozier, Tom Hammick, Georgia Keeling, Helen Turner, Humphrey Ocean, Julian Bell, Craigie Aitchison, Mark Wright, Ken Kiff, Matthew Burrows, Andrzej Jackowski, Sarah Raphael, Nick Bodimeade, Nick Carrick, Mary Newcomb, Hurvin Anderson, Peter Doig, Phoebe Unwin, Danny Markey, Sara Lee, Simon Burton, Susie Hamilton, Marc Chagall, Alfred Wallis, Emil Nolde, J.M.W. Turner, Prunella Clough, Samuel Palmer, Louise Bourgeois, Caspar David Friedrich, Alex Katz, Ewan Gibbs, Susie Hamilton, Andrzej Jackowski, Amanda Vesey, Edward Stott, Gertrude Hermes, Rose Wylie, Sidney Nolan, John Constable, J.M.W. Turner, Emil Nolde, Hiroshige, Edvard Munch, Samuel Palmer, Eileen Cooper, Charles Neame-Spencer, Samantha Cary.

Nuclei of Nearby Active Galaxies: NIR and Sub-mm Views and Finalizing the LINC-NIRVANA Fringe and Flexure Tracking System: Flexure and Temperature Behavior

The work presented in my thesis addresses the two cornerstones of modern astronomy: Observation and Instrumentation. Part I deals with the observation of two nearby active galaxies, the Seyfert 2 galaxy NGC 1433 and the Seyfert 1 galaxy NGC 1566, both at a distance of $\sim10$ Mpc, which are part of the Nuclei of Galaxies (NUGA) sample. It is well established that every galaxy harbors a super massive black hole (SMBH) at its center. Furthermore, there seems to be a fundamental correlation between the stellar bulge and SMBH masses. Simulations show that massive feedback, e.g., powerful outflows, in Quasi Stellar Objects (QSOs) has an impact on the mutual growth of bulge and SMBH. Nearby galaxies follow this relation but accrete mass at much lower rates. This gives rise to the following questions: Which mechanisms allow feeding of nearby Active Galactic Nuclei (AGN)? Is this feeding triggered by events, e.g., star formation, nuclear spirals, outflows, on $\sim500$ pc scales around the AGN? Does feedback on these scales play a role in quenching the feeding process? Does it have an effect on the star formation close to the nucleus? To answer these questions I have carried out observations with the Spectrograph for INtegral Field Observation in the Near Infrared (SINFONI) at the Very Large Telescope (VLT) situated on Cerro Paranal in Chile. I have reduced and analyzed the recorded data, which contain spatial and spectral information in the H-band ($1.45 \mic-1.85 \mic$) and K-band ($1.95 \mic-2.45 \mic$) on the central $10\arcsec\times10\arcsec$ of the observed galaxies. Additionally, Atacama Large Millimeter/Sub-millimeter Array (ALMA) data at $350$ GHz ($\sim0.87$ mm) as well as optical high resolution Hubble Space Telescope (HST) images are used for the analysis. For NGC 1433 I deduce from comparison of the distributions of gas, dust, and intensity of highly ionized emission lines that the galaxy center lies $\sim70$ pc north-northwest of the prior estimate. A velocity gradient is observed at the new center, which I interpret as a bipolar outflow, a circum nuclear disk, or a combination of both. At least one dust and gas arm leads from a $r\sim200$ pc ring towards the nucleus and might feed the SMBH. Two bright warm H$_2$ gas spots are detected that indicate hidden star formation or a spiral arm-arm interaction. From the stellar velocity dispersion (SVD) I estimate a SMBH mass of $\sim1.74\times10^7$ \msol. For NGC 1566 I observe a nuclear gas disk of $\sim150$ pc in radius with a spiral structure. I estimate the total mass of this disk to be $\sim5.4\times10^7$ \msol. What mechanisms excite the gas in the disk is not clear. Neither can the existence of outflows be proven nor is star formation detected over the whole disk. On one side of the spiral structure I detect a star forming region with an estimated star formation rate of $\sim2.6\times10^{-3}$ \msol\ yr$^{-1}$. From broad Br$\gamma$ emission and SVD I estimate a mean SMBH mass of $\sim5.3\times10^6$ \msol\ with an Eddington ratio of $\sim2\times10^{-3}$. Part II deals with the final tests of the Fringe and Flexure Tracker (FFTS) for LBT INterferometric Camera and the NIR/Visible Adaptive iNterferometer for Astronomy (LINC-NIRVANA) at the Large Binocular Telescope (LBT) in Arizona, USA, which I conducted. The FFTS is the subsystem that combines the two separate beams of the LBT and enables near-infrared interferometry with a significantly large field of view. The FFTS has a cryogenic system and an ambient temperature system which are separated by the baffle system. I redesigned this baffle to guarantee the functionality of the system after the final tests in the Cologne cryostat. The redesign did not affect any scientific performance of LINC-NIRVANA. I show in the final cooldown tests that the baffle fulfills the temperature requirement and stays $<110$ K whereas the moving stages in the ambient system stay $>273$ K, which was not given for the old baffle design. Additionally, I test the tilting flexure of the whole FFTS and show that accurate positioning of the detector and the tracking during observation can be guaranteed.

Receptors, sparks and waves in a fire-diffuse-fire framework for calcium release

Calcium ions are an important second messenger in living cells. Indeed calcium signals in the form of waves have been the subject of much recent experimental interest. It is now well established that these waves are composed of elementary stochastic release events (calcium puffs or sparks) from spatially localised calcium stores. The aim of this paper is to analyse how the stochastic nature of individual receptors within these stores combines to create stochastic behaviour on long timescales that may ultimately lead to waves of activity in a spatially extended cell model. Techniques from asymptotic analysis and stochastic phase-plane analysis are used to show that a large cluster of receptor channels leads to a release probability with a sigmoidal dependence on calcium density. This release probability is incorporated into a computationally inexpensive model of calcium release based upon a stochastic generalization of the Fire-Diffuse-Fire (FDF) threshold model. Numerical simulations of the model in one and two dimensions (with stores arranged on both regular and disordered lattices) illustrate that stochastic calcium release leads to the spontaneous production of calcium sparks that may merge to form saltatory waves. Illustrations of spreading circular waves, spirals and more irregular waves are presented. Furthermore, receptor noise is shown to generate a form of array enhanced coherence resonance whereby all calcium stores release periodically and simultaneously.

Study of the behavior of iron ore particles in spiral concentrators

Les spirales sont des appareils de séparation gravimétrique principalement utilisés dans l’industrie du traitement du minerai de fer. La classification des particules dans la pulpe s’effectue lors de la descente dans les spires en fonction de leur taille et leur densité, des conditions d’opération et de la géométrie de la spirale. L’effet des conditions d’opération (pourcentage solide, débit d’alimentation et débit d’eau de lavage) est évalué sur la performance des spirales en utilisant une spirale WW6E installée à COREM pour traiter un minerai de fer de ArcelorMittal, Québec. Les résultats montrent l’effet dominant du débit de l’eau de lavage et son impact majeur sur les particules grossières. Un circuit fermé de trois spirales parallèles avec 3, 5 et 7 tours est utilisé afin d’évaluer l’influence du nombre de tours. Les résultats préliminaires indiquent que la spirale trois tours fonctionne bien pour le nettoyage tandis que la 7 tour est robuste pour l’ébauchage et l’épuisage.

Some results on open-edge and open mobile guarding of polygons and triangulations

This paper focuses on a variation of the Art Gallery problem that considers open-edge guards and open mobile-guards. A mobile guard can be placed on edges and diagonals of a polygon, and the ‘open’ prefix means that the endpoints of such an edge or diagonal are not taken into account for visibility purposes. This paper studies the number of guards that are sufficient and sometimes necessary to guard some classes of simple polygons for both open-edge and open mobile-guards. A wide range of polygons is studied, which include orthogonal polygons with or without holes, spirals, orthogonal spirals and monotone polygons. Moreover, this problem is also considered for planar triangulation graphs using open-edge guards.

Projeto, construção e análise de um prototipo vibracional em escala de bancada aplicável ao tratamento de água de produção de petróleo bruto, mediante inovadora operação híbrida de adsorção e auto-flotação

A self-flotator vibrational prototype electromechanical drive for treatment of oil and water emulsion or like emulsion is presented and evaluated. Oil production and refining to obtain derivatives is carried out under arrangements technically referred to as on-shore and off-shore, ie, on the continent and in the sea. In Brazil 80 % of the petroleum production is taken at sea and area of deployment and it cost scale are worrisome. It is associated, oily water production on a large scale, carrier 95% of the potential pollutant of activity whose final destination is the environment medium, terrestrial or maritime. Although diversified set of techniques and water treatment systems are in use or research, we propose an innovative system that operates in a sustainable way without chemical additives, for the good of the ecosystem. Labyrinth adsor-bent is used in metal spirals, and laboratory scale flow. Equipment and process patents are claimed. Treatments were performed at different flow rates and bands often monitored with control systems, some built, other bought for this purpose. Measurements of the levels of oil and grease (OGC) of efluents treaty remained within the range of legal framework under test conditions. Adsorbents were weighed before and after treatment for obtaining oil impregna-tion, the performance goal of vibratory action and treatment as a whole. Treatment technolo-gies in course are referenced, to compare performance, qualitatively and quantitatively. The vibration energy consumption is faced with and without conventional flotation and self-flotation. There are good prospects for the proposed, especially in reducing the residence time, by capillary action system. The impregnation dimensionless parameter was created and confronted with consecrated dimensionless parameters, on the vibrational version, such as Weber number and Froude number in quadratic form, referred to as vibrational criticality. Re-sults suggest limits to the vibration intensity

Lieu de liens, lieu de vie : oser le réseau comme alternative à la vulnérabilité : le cas des demandeurs d’asile à Projet Refuge (Montréal).

La vulnérabilité est l’attribut fondamental justifiant le passage des frontières du refuge canadien (Rousseau et al., 2002 ; Clément et Bolduc, 2004). Elle est preuve d’insécurité pour la victime requérant l’asile ; elle est aussi porteuse d’espérance de sécurité en terre hospitalière. Elle est pourtant potentiel réactualisé dans l’insécurité d’un statut incertain en terre d’accueil (Agamben, 1997 ; D’Halluin, 2004). Violente immersion. En attendant que les preuves de sa vulnérabilité originelle soient validées, le demandeur d’asile se retrouve dans un entre-deux a-territorial et atemporel (Agier, 2002 ; Le Blanc, 2010) et dans une précarité tout aussi dangereuse (Ouimet et al., 2009). Des besoins émergent en cette terre inconnue, or l’accès aux soins de santé lui est limité par des textes de lois ambigus et leurs interprétations maladroites (Harris et Zuberi, 2015). Ainsi lorsqu’il se heurte à des barrières érigées par une transmission d’informations défectueuse, sa précarité ne fait qu’empirer. Tel un boomerang, ce paradoxe cultive leur vulnérabilité. Alors que les recherches interrogent les divers intervenants en santé (Asgary et Smith, 2013), j’ai choisi de donner la parole aux premiers concernés et de relayer leur vécu par rapport à leur propre personne. Deux objectifs principaux guident la recherche : documenter dans un premier temps leur parcours de quête de soins à partir de la circulation des informations formelles et informelles dans le but de sonder leur avis sur la vulnérabilité qui leur est attribuée ; documenter dans un second temps leur parcours migratoire de quête de soi afin de mettre en lumière les stratégies alternatives d’entrée en contact avec la société d’accueil pour négocier voire rejeter cette identité vulnérable. J’ai rencontré pour cela des demandeurs d’asile lors d’un terrain de huit mois au sein d’un organisme communautaire d’hébergement à Montréal. Dans ce contexte d’accompagnement et de stabilité spatiale, accalmie bienvenue au terme d’un itinéraire semé d’embûches, les ressources informationnelles sont à leur disposition et la reconnaissance sociale est à l’honneur. En parallèle, beaucoup témoignent de la diminution de leurs besoins de soins de santé. En cette communauté thérapeutique (Pocreau, 2005), véritable tremplin vers la société d’accueil en attendant un statut reconnu, ils bénéficient d’une possibilité de participation sociale et d’un sentiment d’appartenance valorisant. Si des conditions précaires peuvent aggraver la vulnérabilité, le bricolage de conditions positives favorise la résilience (Cleveland et al., 2014), créant un environnement revitalisant qui leur permet de rebondir.

Lieu de liens, lieu de vie : oser le réseau comme alternative à la vulnérabilité : le cas des demandeurs d’asile à Projet Refuge (Montréal)

La vulnérabilité est l’attribut fondamental justifiant le passage des frontières du refuge canadien (Rousseau et al., 2002 ; Clément et Bolduc, 2004). Elle est preuve d’insécurité pour la victime requérant l’asile ; elle est aussi porteuse d’espérance de sécurité en terre hospitalière. Elle est pourtant potentiel réactualisé dans l’insécurité d’un statut incertain en terre d’accueil (Agamben, 1997 ; D’Halluin, 2004). Violente immersion. En attendant que les preuves de sa vulnérabilité originelle soient validées, le demandeur d’asile se retrouve dans un entre-deux a-territorial et atemporel (Agier, 2002 ; Le Blanc, 2010) et dans une précarité tout aussi dangereuse (Ouimet et al., 2009). Des besoins émergent en cette terre inconnue, or l’accès aux soins de santé lui est limité par des textes de lois ambigus et leurs interprétations maladroites (Harris et Zuberi, 2015). Ainsi lorsqu’il se heurte à des barrières érigées par une transmission d’informations défectueuse, sa précarité ne fait qu’empirer. Tel un boomerang, ce paradoxe cultive leur vulnérabilité. Alors que les recherches interrogent les divers intervenants en santé (Asgary et Smith, 2013), j’ai choisi de donner la parole aux premiers concernés et de relayer leur vécu par rapport à leur propre personne. Deux objectifs principaux guident la recherche : documenter dans un premier temps leur parcours de quête de soins à partir de la circulation des informations formelles et informelles dans le but de sonder leur avis sur la vulnérabilité qui leur est attribuée ; documenter dans un second temps leur parcours migratoire de quête de soi afin de mettre en lumière les stratégies alternatives d’entrée en contact avec la société d’accueil pour négocier voire rejeter cette identité vulnérable. J’ai rencontré pour cela des demandeurs d’asile lors d’un terrain de huit mois au sein d’un organisme communautaire d’hébergement à Montréal. Dans ce contexte d’accompagnement et de stabilité spatiale, accalmie bienvenue au terme d’un itinéraire semé d’embûches, les ressources informationnelles sont à leur disposition et la reconnaissance sociale est à l’honneur. En parallèle, beaucoup témoignent de la diminution de leurs besoins de soins de santé. En cette communauté thérapeutique (Pocreau, 2005), véritable tremplin vers la société d’accueil en attendant un statut reconnu, ils bénéficient d’une possibilité de participation sociale et d’un sentiment d’appartenance valorisant. Si des conditions précaires peuvent aggraver la vulnérabilité, le bricolage de conditions positives favorise la résilience (Cleveland et al., 2014), créant un environnement revitalisant qui leur permet de rebondir.

Como podem as organizações gerir paradoxos?

As organizações participam em ambientes que, além de complexos, são repletos de ambiguidade e de exigências contraditórias. A capacidade de trabalhar com os paradoxos é necessária para responder a essa complexidade ambiental. Este artigo discute como esse desafio pode ser levado a cabo. Começa por esclarecer a diferença entre processos por vezes equiparados a paradoxos por envolverem contradições, nomeadamente dilemas e dialéticas. Trata, depois, de diferentes possibilidades de resposta às situações paradoxais. Discute, finalmente, como dessas respostas podem resultar círculos viciosos versus virtuosos.