ALMA Reveals Sequential High-mass Star Formation in the G9.62+0.19 Complex-Reference-Cited by-同舟云学术

ALMA Reveals Sequential High-mass Star Formation in the G9.62+0.19 Complex

Published:2017-10-26 Issue:1 Volume:849 Page:25
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Liu Tie^ORCID,Lacy John^ORCID,Li Pak Shing,Wang Ke^ORCID,Qin Sheng-Li^ORCID,Zhang Qizhou^ORCID,Kim Kee-Tae^ORCID,Garay Guido,Wu Yuefang,Mardones Diego^ORCID,Zhu Qingfeng^ORCID,Tatematsu Ken’ichi^ORCID,Hirota Tomoya^ORCID,Ren Zhiyuan,Liu Sheng-Yuan^ORCID,Chen Huei-Ru^ORCID,Su Yu-Nung,Li Di

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/849/i=1/a=25/pdf

Reference97 articles.

1. From filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from theHerschelGould Belt Survey

2. Star formation through gravitational collapse and competitive accretion

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