Simulating protostellar evolution and radiative feedback in the cluster environment

Abstract. Radiative feedback is among the most important consequences of clustered star formation inside molecular clouds. At the onset of star formation, radi

Saved in:
Bibliographic Details
Main Authors: Klassen, Mikhail (Author) , Pudritz, Ralph E. (Author) , Peters, Thomas (Author)
Format: Article (Journal)
Language:English
Published: 10 April 2012
In: Monthly notices of the Royal Astronomical Society
Year: 2012, Volume: 421, Issue: 4, Pages: 2861-2871
ISSN:1365-2966
DOI:10.1111/j.1365-2966.2012.20523.x
Online Access:Verlag, Volltext: http://dx.doi.org/10.1111/j.1365-2966.2012.20523.x
Verlag, Volltext: https://academic.oup.com/mnras/article/421/4/2861/1085345
Get full text
Author Notes:Mikhail Klassen, Ralph E. Pudritz, Thomas Peters
Description
Summary:Abstract. Radiative feedback is among the most important consequences of clustered star formation inside molecular clouds. At the onset of star formation, radi
Item Description:Gesehen am 05.02.2019
Physical Description:Online Resource
ISSN:1365-2966
DOI:10.1111/j.1365-2966.2012.20523.x