The H II Region G333.6-0.2, a Very Powerful 1-20 Micron Source-Reference-Cited by-同舟云学术

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The H II Region G333.6-0.2, a Very Powerful 1-20 Micron Source

Published:1973-06 Issue: Volume:182 Page:L125
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Becklin E. E.,Frogel J. A.,Neugebauer G.,Persson S. E.,Wynn-Williams C. G.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 44 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. Infall, outflow, and turbulence in massive star-forming cores in the G333 giant molecular cloud;Monthly Notices of the Royal Astronomical Society;2015-09-04

2. TRACING H 2 COLUMN DENSITY WITH ATOMIC CARBON (C I) AND CO ISOTOPOLOGS;The Astrophysical Journal;2014-12-03

3. Molecular line mapping of the giant molecular cloud associated with RCW 106 – IV. Ammonia towards dust emission;Monthly Notices of the Royal Astronomical Society;2014-04-24

4. Radiatively driven Rayleigh-Taylor instability candidates around a forming massive star system;Astronomy & Astrophysics;2013-10

5. Spectrophotometric distances to Galactic H ii regions;Monthly Notices of the Royal Astronomical Society;2010-11-25

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