Ruprecht-Karls-Universität Heidelberg

Vortragsdetails

Montag, 10. Oktober 2011 - 11:00

Rowan Smith:

"Understanding the dynamics of star formation"

Zusammenfassung. Star formation regions are complex regions where both turbulence and self-gravity cause molecular clouds to collapse into dense filaments and cores. In this talk I will show how such complex motions are translated into observed line profiles, and look at how we can use simulations to help us gain a deeper understanding of the observed dynamics of star formation.

Verantwortlich: , letzte Änderung am 05.04.2013 11:50 CEST
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