Wine and Cheese Spring 2018: Difference between revisions

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=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)

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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

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February 26th

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March 5th

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March 12th (Graduate Student Series)

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March 19th

Spring Break

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March 26th

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April 2nd

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April 9th

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April 16th

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April 23rd (Graduate Student Series)

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