Simulations of the star-forming molecular gas in an interacting M51-like galaxy

ABSTRACT. We present here the first of a series of papers aimed at better understanding the evolution and properties of giant molecular clouds (GMCs) in a gala

Saved in:
Bibliographic Details
Main Authors: Treß, Robin G. (Author) , Sormani, Mattia C. (Author) , Glover, Simon (Author) , Klessen, Ralf S. (Author)
Format: Article (Journal)
Language:English
Published: 2020 January 09
In: Monthly notices of the Royal Astronomical Society
Year: 2020, Volume: 492, Issue: 2, Pages: 2973-2995
ISSN:1365-2966
DOI:10.1093/mnras/stz3600
Online Access:Verlag, Volltext: https://doi.org/10.1093/mnras/stz3600
Verlag: https://academic.oup.com/mnras/article/492/2/2973/5698815
Get full text
Author Notes:Robin G. Tress, Rowan J. Smith, Mattia C. Sormani, Simon C.O. Glover, Ralf S. Klessen, Mordecai-Mark Mac Low and Paul C. Clark
Description
Summary:ABSTRACT. We present here the first of a series of papers aimed at better understanding the evolution and properties of giant molecular clouds (GMCs) in a gala
Item Description:Gesehen am 17.02.2020
Physical Description:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/stz3600