HCO+ in NGC 6334

Author:

Batchelor R. A.,Robinson B. J.,McCulloch M. G.

Abstract

In this paper we present maps showing the distribution of HCO+ (J= 1→0 transition at 89.18855 GHz) in the direction of NGC 6334 as a function of radial velocity, lhe observations were carried out in May-June 1979 as part of a larger program of HCO+ observations (Batchelor et al. 1980, 1981) using the Epping 4-m millimetre-wave radio telescope.

Publisher

Cambridge University Press (CUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 7 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. The global velocity field of the filament in NGC 6334;Astronomy & Astrophysics;2013-06

2. Properties of the Photodissociated Gas in NGC 6334;The Astrophysical Journal;2000-10-20

3. Molecular Gas in the NGC 6334 Star Formation Region;The Astrophysical Journal Supplement Series;1999-10

4. Studies of dense molecular cores in regions of massive star formation. IV. Multitransition CS-study towards;Astronomy and Astrophysics Supplement Series;1996-08

5. Ionized Carbon in NGC 6334;The Astrophysical Journal;1995-11

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