The dynamical evolution of molecular clouds near the Galactic Centre: II. Spatial structure and kinematics of simulated clouds

ABSTRACT. The evolution of molecular clouds in galactic centres is thought to differ from that in galactic discs due to a significant influence of the external

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Bibliographic Details
Main Authors:	Kruijssen, Diederik (Author) , Jeffreson, Sarah (Author) , Petkova, Maya A. (Author)
Format:	Article (Journal)
Language:	English
Published:	2019 February 7
In:	Monthly notices of the Royal Astronomical Society Year: 2019, Volume: 484, Issue: 4, Pages: 5734-5754
ISSN:	1365-2966
DOI:	10.1093/mnras/stz381
Online Access:	Verlag, Volltext: http://dx.doi.org/10.1093/mnras/stz381 Verlag, Volltext: https://academic.oup.com/mnras/article/484/4/5734/5308852
Author Notes:	J.M.D. Kruijssen, J.E. Dale, S.N. Longmore, D.L. Walker, J.D. Henshaw, S.M.R. Jeffreson, M.A. Petkova, A. Ginsburg, A.T. Barnes, C.D. Battersby, K. Immer, J.M. Jackson, E.R. Keto, N. Krieger, E.a.C. Mills, Á. Sánchez-Monge, A. Schmiedeke, S.T. Suri and Q. Zhang

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Summary:	ABSTRACT. The evolution of molecular clouds in galactic centres is thought to differ from that in galactic discs due to a significant influence of the external
Item Description:	Gesehen am 04.03.2019
Physical Description:	Online Resource
ISSN:	1365-2966
DOI:	10.1093/mnras/stz381