Stellar & AGN Feedback in Galaxies GLCW8 Columbus 2007.
OBJECTIVES: 1.Know the phases of star formation starting with the interstellar cloud. 2.Understand how the life cycle of both low and high mass stars contribute.
EGOs: Massive YSOs in IRDCs Ed Churchwell & Claudia Cyganowski with co-workers: Crystal Brogan, Todd Hunter, Barb Whitney Qizhou Zhang Dense Cores in Dark.
In a dense molecular cloud far, far away M16: The Eagle Nebula Dense Molecular gas Hot, ionized gas Young stars.
Chaotic Case Studies: Sensitive dependence on initial conditions in star/planet formation Fred C. Adams Physics Department University of Michigan With:
Stellar & AGN Feedback in Galaxies
