Wine and Cheese Spring 2018: Difference between revisions
No edit summary |
|||
Line 14: | Line 14: | ||
=February 12th= | =February 12th= | ||
== == | == Amiel Sternberg== | ||
'''-'''<br> | '''The Atomic to Molecular (HI-to-H2) Transition in Galaxy Star-Forming Regions'''<br> | ||
The atomic to molecular hydrogen (HI-to-H2) phase transition is of fundamental importance for star-formation and the emergence of chemical complexity in the interstellar medium of galaxies. I will present an overview, and discuss recent theoretical studies, numerical and analytic, of the HI-to-H2 transition in irradiated systems, with applications to the multi-scale behavior observed in star-forming galaxy disks from low- to high-redshift. | |||
=February 19th= | =February 19th= |
Revision as of 19:02, 2 February 2018
This page records the schedule, titles and abstracts of the JHU/STScI CAS Astrophysics Wine & Cheese Series in Fall 2017.
Wine and Cheese sessions with one talk will have a 50 minute talk with 10 minutes for questions. Sessions with two speakers will have two 25 minute talks, each with 5 minutes for questions. Sessions in the Graduate Student Series will have three 15 minute talks, each with 5 minutes for questions.
Back to W&C Schedule
February 5th (Graduate Student Series)
-
February 12th
Amiel Sternberg
The Atomic to Molecular (HI-to-H2) Transition in Galaxy Star-Forming Regions
The atomic to molecular hydrogen (HI-to-H2) phase transition is of fundamental importance for star-formation and the emergence of chemical complexity in the interstellar medium of galaxies. I will present an overview, and discuss recent theoretical studies, numerical and analytic, of the HI-to-H2 transition in irradiated systems, with applications to the multi-scale behavior observed in star-forming galaxy disks from low- to high-redshift.
February 19th
-
February 26th
-
March 5th
-
March 12th (Graduate Student Series)
-
March 19th
Spring Break
-
March 26th
-
April 2nd
-
April 9th
-
April 16th
-
April 23rd (Graduate Student Series)
-