The first hyper_luminous_infrared_galaxy_discovered_by_wise
Kathryn wheel a_spectacular_galaxy_collision_discoverd_in_the_galactic_neighbourhood
The Cosmic Near-Infrared Background: Remnant light form early stars Journal Club talk 3.12.2010 A. B. Fry Ferdinand & Komatsu 2006 (F&K06) also Ferdinand.
Deep Neutral Hydrogen Surveys with the Arecibo 305-m Telescope – the Arecibo Galaxy Environment Survey Robert Minchin NAIC Arecibo Observatory. [email protected].
STAR FORMATION In honor of Yakov B. Zeldovich Moscow June 20, 2014 Chris McKee.
I. Old dwarf starburst galaxies in the local Universe: Blue Compact Dwarf Galaxies (BCDs) - general properties - the star-forming component - open questions.
HI Gas as Function of Environment When and where do galaxies stop accreting cool gas? How do they loose the cool gas? When do they stop forming stars?
Hello!. Ajit Kembhavi IUCAA, Pune Galaxies Near and Far Galaxy Morphology, SuperMassive Black Holes and all that Sudhanshu Barway Yogesh Wadadekar Vinu.
Eric M. Wilcots University of Wisconsin-Madison. How and when did galaxies accrete their gas? Where and when did/do galaxies stop accreting gas?
The Prevalence and Properties of Outflowing Galactic Winds at z = 1 Katherine A. Kornei (UCLA) Alice E. Shapley (UCLA) Crystal L. Martin (UCSB) Alison.
SFR and COSMOS Bahram Mobasher + the COSMOS Team.
Submillimeter and IR Studies of Molecular Regions in the Magellanic Clouds Mónica Rubio Universidad de Chile CCAT Workshop, Koln, 5oct11.