Saturday. Here begins my daily prayer (11:46 am). Daily prayers at the beginning of the day (i.e., 6am) is better, as I did yesterday.
MPIfR Lunch Colloquium
MPIfR 0.02, Sept 28, 13:00
Structure of hot molecular cores
Rainer Rolffs
Hot molecular cores: transient phase of high-mass star formation (heated up, but before being ionized). Intro to high-mass star formation; present observation (APEX/Herschel, VLA/SMA) and analysis (spherical radiative transfer and 3-d modeling) methods; highlight results. Mass of hot molecular gas, internal heating mechanism (radiation diffusion), infall reversal in the central region, centrally flat density distribution. All can be explained by increased central pressure caused by feedback from young massive stars in a high-column-density environment.
AIfA Master-Kolloquium
AIfA 0.012, 29 Sept. 2011, 11:00
Constraints on the "Universal" Pressure Profile through the SZ power spectrum
Miriam Elizabeth Ramos Ceja
* I've read this one before.
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