Star Formation in the Sh 2-53 Region Influenced by Accreting Molecular Filaments-Reference-Cited by-同舟云学术

Star Formation in the Sh 2-53 Region Influenced by Accreting Molecular Filaments

Published:2018-01-15 Issue:2 Volume:852 Page:119
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Baug T.^ORCID,Dewangan L. K.^ORCID,Ojha D. K.^ORCID,Tachihara Kengo^ORCID,Pandey A. K.,Sharma Saurabh^ORCID,Tamura M.^ORCID,Ninan J. P.^ORCID,Ghosh S. K.^ORCID

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/852/i=2/a=119/pdf

Reference71 articles.

1. RESOLUTION OF THE DISTANCE AMBIGUITY FOR GALACTIC H II REGIONS

2. Characterizing filaments in regions of high-mass star formation: High-resolution submilimeter imaging of the massive star-forming complex NGC 6334 with ArTéMiS

3. Sh2-138: physical environment around a small cluster of massive stars

4. GLIMPSE. I. AnSIRTFLegacy Project to Map the Inner Galaxy

5. Catalog of CO radial velocities toward galactic H II regions

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