Artigo Acesso aberto Revisado por pares

NGC 6334 and NGC 6357: H α kinematics and the nature of the H II regions

2016; EDP Sciences; Volume: 587; Linguagem: Inglês

10.1051/0004-6361/201424484

ISSN

1432-0746

Autores

D. Russeil, J. Tigé, C. Adami, L. D. Anderson, N. Schneider, A. Zavagno, M. R. Samal, P. Amram, L. Guennou, E. Le Coarer, Andrew Walsh, S. N. Longmore, Cormac Purcell,

Tópico(s)

Astronomy and Astrophysical Research

Resumo

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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