'Accretion rates' diaporamas de présentation

Stellar Rotation: A Probe of Star-Forming Modes and Initial Conditions?

Stellar Rotation: A Probe of Star-Forming Modes and Initial Conditions?. Sidney C. Wolff and Stephen E. Strom National Optical Astronomy Observatory (With collaborators Luisa Rebull, Kim Venn, and REU students David Dror and Laura Kushner). Motivation. Address two key questions:

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The Build-up of Quasars

The Build-up of Quasars. Gordon Richards Drexel University. With thanks to Michael Strauss, Yue Shen (Princeton), Don Schneider, Nic Ross (Penn State), Adam Myers (Illinois ), Phil Hopkins ( Berkeley ), and a host of other people from the SDSS Collaboration. Caveats.

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How do massive stars form ? A comparison of model tracks with Herschel data

How do massive stars form ? A comparison of model tracks with Herschel data. Michael D Smith CAPS University of Kent Available at: http://astro.kent.ac.uk/mds/capsule.pdf September 2013. L ate stage: Rosette in optical . AFGL 2591. Rosette Nebula, Travis Rector, KPNO.

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Molecular absorption in Cen A on VLBI scales

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OSTEOPENIA OF PREMATURITY

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OSTEOPENIA OF PREMATURITY

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Neutron Stars 3: Thermal evolution

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The complex and puzzling phenomenology of thermonuclear X-ray bursts

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Project Level Effectiveness Monitoring in the Estuary and Response in Fish Communities

Project Level Effectiveness Monitoring in the Estuary and Response in Fish Communities. Who is CREST?. Council of Governments (b. 1974)

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Results from AGN multiple wavelength observations and the importance of monitoring campaigns

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Non-HBLR S2 and Unified Model of AGNs

Non-HBLR S2 and Unified Model of AGNs. Zhang Enpeng Wang Jianmin 04. 22. 2006. Outline. Introduction Data and analysis Conclusion. I Introduction Carl Seyfert (1943) ( --- Seyfert galaxies)

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UNCERTAINTIES ON THE BLACK HOLE MASSES AND CONSEQUENCES FOR THE EDDINGTON RATIOS Suzy Collin

UNCERTAINTIES ON THE BLACK HOLE MASSES AND CONSEQUENCES FOR THE EDDINGTON RATIOS Suzy Collin Observatoire de Paris-Meudon, France Collaborators: T. Kawaguchi (Tokyo), B. Peterson (Ohio U), M. Vestergaard (Steward obs), C. Boisson, M. Mouchet (Paris).

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CIV Emission as a Probe of Accretion Disk Winds

CIV Emission as a Probe of Accretion Disk Winds. Gordon Richards Drexel University. With thanks to Sarah Gallagher (UWO), Karen Leighly (OU), Paul Hewett ( IoA , Cambridge), and Nick Kruczek , Rachael Kratzer , and Coleman Krawczyk (Drexel). Clouds (and Torus?) => Disk Winds.

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Transient X-ray Binaries in the Galactic Center

Transient X-ray Binaries in the Galactic Center. Michael Muno (Caltech). A Brief Introduction to X-ray Binaries. RXTE ASM. Monitoring X-ray Binaries. Are disk-fed. Accretion is unstable at low mass transfer rates. Neutron stars produce thermonuclear bursts. Are wind-fed.

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Luminous Hot Accretion Flows

Luminous Hot Accretion Flows. ------extending ADAF beyond its critical accretion rate. Feng Yuan Shanghai Astronomical Observatory, Chinese Academy of Science. Outline. The dynamics of luminous hot accretion flows (LHAFs) Main features of LHAFs Stability

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Black Hole Masses and accretion rates

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Dispersal of protoplanetary disks by central wind stripping

Dispersal of protoplanetary disks by central wind stripping. Isamu Matsuyama University of California Berkeley David Hollenbach SETI Institute Doug Johnstone Herzberg Institute of Astrophysics.

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The Growth of the Stellar Seeds of Supermassive Black Holes

The Growth of the Stellar Seeds of Supermassive Black Holes. Jarrett Johnson (LANL, MPE) with Bhaskar Agarwal (MPE), Claudio Dalla Vecchia (MPE), Fabrice Durier ( Victoria,MPE ), Chris Fryer (LANL), Thomas Greif (MPA), Sadegh Khochfar (MPE), Hui Li (LANL), and Dan Whalen (CMU, LANL).

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Unusual radio BAL quasar 1624+3758

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