Chapter i
Observations of the evolution of HI in galaxies across different environments. D.J. Pisano (West Virginia University)
1 Steve Lord & Joseph Mazzarella (here in spirit): Extreme Starbursts, Lijiang China, 14-18 August 2005 Part I: Our Spitzer Imaging Program of a Complete.
The M-81 Group of Galaxies Brian Fleming Stephanie LaMassa Seamus Riley (The Chunky Ponies)
Image Credit: NASA,ESA and the Hubble SM4 ERO Team Michelle Cluver [email protected].
SFR and COSMOS Bahram Mobasher + the COSMOS Team.
Disentangling Luminosity, Morphology, Stellar Age, Star Formation, and Environment in Galaxy Evolution Daniel Christlein Andes Fellow Yale University.
I N T R O D U C T I O N The mechanism of galaxy formation involves the cooling and condensation of baryons inside the gravitational potential well provided.
Observations of the evolution of HI in galaxies across different environments.
Future modelling efforts Eelco van Kampen ESO [email protected].
The PSI Planet-building Code: Multi-zone, Multi-use S. J. Weidenschilling PSI Retreat August 20, 2007.
The moon and the earth’s rotation rate
