A simple model to explain the high gas content of galaxy UGC 8802 Ruixiang Chang Shanghai Astronomical Observatory Collaborators: Jinliang Hou Shiyin Shen.
Two Phase Formation of Massive Galaxies T.Naab, P. Johansson, R. Cen, K. Nagamine, R. Joung and J.P.O. PPPL:, 19 Dec 2012 ApJ.L.,658,710 (2007) ApJ.,697,
Dynamical Models James Binney Oxford University. Outline Importance of models Importance of models Modelling methods Modelling methods Schoenrich’s model.
Hunt for Molecules in Local Universe Galaxies Santiago GARCIA-BURILLO Observatorio Astronómico Nacional (OAN)-Spain Hunt for Molecules, November 19-20,
DARS, October 9, 2008 Chemical evolution in the MW Observational evidence Birgitta Nordström Niels Bohr Institute.
Radio galaxies: timescales and triggers Elaine Sadler, University of Sydney Goal: To develop a self-consistent picture of how radio galaxies are triggered,
NUclei of GAlaxies: First results of NUGA Santiago GARCIA BURILLO ([email protected]) Observatorio Astronómico Nacional (OAN) The NUGA project People involved.
8th Sino-German Workshop Kunming, Feb 23-28, 2009 Milky Way vs. M31: a Tale of Two Disks Jinliang HOU In collaboration with : Ruixiang CHANG, Shiyin SHEN,
Musings about 30 Dor
The merging history of dark halos dominates galaxy formation. Spiral galaxies: merging of small, gas-rich substructures. Elliptical Galaxies: merging of.
Musings about 30 Dor Hans Zinnecker DSI @ SOFIA Science Center NASA-Ames Research Center Moffett Field, CA (Univ. Stuttgart, Germany)
Front
