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NGC 6334 and NGC 6357: Hαkinematics and the nature of the H II regions
Authors
D. Russeil,J. Tigé
C. Adami,L. D. Anderson,N. Schneider,A. Zavagno,M. R. Samal,P. Amram,L. Guennou,E. Le Coarer,A. Walsh,S. N. Longmore,C. Purcell,L. Anderson,M. Samal,E. Coarer,Steven Longmore
+15 authors
,Cormac PurcellJournal
Published
Mar 1, 2016
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Abstract
Aims. NGC 6334 and NGC 6357 are amongst the most active, optically visible Galactic star-forming complexes. They are composed of several H ii regions that have a significant impact on their surrounding. The aim of this paper is to present a kinematic study of the optical H ii regions that belong to NGC 6334 and NGC 6357.
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