'Stellar disks' diaporamas de présentation

HI Gas as Function of Environment

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?. Jen Donovan poster. The lore.. if halos get too big, gas does not cool But.. at least some dry mergers are wet, and forming stars

461 views • 35 slides

James Wadsley, Sijing Shen (McMaster) , Lucio Mayer, Joachim Stadel (Zurich) ,Graeme Luftkin (Maryland), Tom Quinn

Simulating the Fragmentation of Proto-planetary disks. UWO Disk Workshop 2006. James Wadsley, Sijing Shen (McMaster) , Lucio Mayer, Joachim Stadel (Zurich) ,Graeme Luftkin (Maryland), Tom Quinn (Washington). Overview.

520 views • 29 slides

350 ? m Observations of Asteroids, Secondary Calibrators, and Stellar Standard(s)

350 ? m Observations of Asteroids, Secondary Calibrators, and Stellar Standard(s). C. Darren Dowell Jet Propulsion Laboratory, California Institute of Technology,USA 2008 Feb 7. Scope of this Project. CSO/SHARC II 350 ? m archive (2003-date):

313 views • 22 slides

Island Universes: Structure and Evolution of Disk Galaxies

317 views • 19 slides

Island Universes: Structure and Evolution of Disk Galaxies

289 views • 19 slides