G331.512–0.103: An Interstellar Laboratory for Molecular Synthesis. I. The Ortho-to-para Ratios for CH3OH and CH3CN-Reference-Cited by-同舟云学术

G331.512–0.103: An Interstellar Laboratory for Molecular Synthesis. I. The Ortho-to-para Ratios for CH3OH and CH3CN

Published:2018-02-01 Issue:2 Volume:853 Page:152
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Mendoza Edgar^ORCID,Bronfman Leonardo^ORCID,Duronea Nicolas U.,Lépine Jacques R. D.^ORCID,Finger Ricardo,Merello Manuel^ORCID,Hervías-Caimapo Carlos,Gama Diana R. G.^ORCID,Reyes Nicolas,Åke-Nyman Lars

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/853/i=2/a=152/pdf

Reference71 articles.

1. CH 3 CN Observations toward Southern Massive Star‐forming Regions

2. A necklace of dense cores in the high-mass star forming region G35.20−0.74 N: ALMA observations

3. Outflow and Dense Gas Emission from Massive Infrared Dark Clouds

4. Line Imaging of Orion KL at 865 μm with the Submillimeter Array

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