DOCUMENT RESOURCES FOR EVERYONE
Documents tagged
Documents Cosmological Structure Formation A Short Course III. Structure Formation in the Non-Linear Regime...

Slide 1Cosmological Structure Formation A Short Course III. Structure Formation in the Non-Linear Regime Chris Power Slide 2 Recap Cosmological inflation provides mechanism…

Documents The main growth modes of disks, bulges, and central black holes: Mergers - Violent Instabilities -.....

Slide 1The main growth modes of disks, bulges, and central black holes: Mergers - Violent Instabilities - Secular Evolution Frédéric Bournaud - CEA Saclay with Stéphanie…

Documents A Deep XMM-Newton Study of the Hot Gaseous Halo Around NGC 1961

Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed 10 August 2015 (MN LATEX style file v2.2) A Deep XMM-Newton Study of the Hot Gaseous Halo Around NGC 1961 Michael…

Documents Effects of galaxy formation on dark matter haloes Susana Pedrosa Patricia Tissera, Cecilia...

Slide 1Effects of galaxy formation on dark matter haloes Susana Pedrosa Patricia Tissera, Cecilia Scannapieco Chile 2010 Slide 2 Introduction Cuspy inner profiles obtained…

Documents DARK MATTER IN GALAXIES Paolo Salucci (SISSA). Dennis: Rotation Curves, Dark Matter, Nature of, Role...

Slide 1DARK MATTER IN GALAXIES Paolo Salucci (SISSA) Slide 2 Dennis: Rotation Curves, Dark Matter, Nature of, Role of Baryons. Importance of the topics but low interest from…

Documents Dec. 1-8, 2010 DARK MATTER IN GALAXIES Alessandro Romeo Onsala Space Observatory Chalmers University...

Slide 1 Dec. 1-8, 2010 DARK MATTER IN GALAXIES Alessandro Romeo Onsala Space Observatory Chalmers University of Technology SE-43992 Onsala, Sweden Slide 2 Overview Dark matter…

Documents Deep Chandra and XMM-Newton Observations of NGC 4472 R. P. Kraft, S. W. Randall, W. R. Forman, P. E....

Slide 1 Deep Chandra and XMM-Newton Observations of NGC 4472 R. P. Kraft, S. W. Randall, W. R. Forman, P. E. J. Nulsen, C. Jones, A. Bogdan, M. J. Hardcastle, E. Hallman,…

Documents Is the Sodium Na D line useful? Marcel Bergmann Bo Milvang-Jensen.

Slide 1 Is the Sodium Na D line useful? Marcel Bergmann Bo Milvang-Jensen Slide 2 Background Galaxies are full of stars, and sometimes gas and dust too. Beyond just images…

Documents With a wide-field multi-IFU spectrograph. Clusters provide large samples of galaxies in a moderate....

Slide 1 With a wide-field multi-IFU spectrograph Slide 2  Clusters provide large samples of galaxies in a moderate field  Unique perspective on the interaction of galaxies…

Documents How Do Galaxies Get Their Gas? astro-ph/0407095 Dušan Kereš University of Massachusetts...

Slide 1 How Do Galaxies Get Their Gas? astro-ph/0407095 Dušan Kereš University of Massachusetts Collaborators: Neal Katz, Umass David Weinberg, Ohio-State Romeel Davé,…