Relationship between CH<sub>3</sub>OD Abundance and Temperature in the Orion KL Nebula-Reference-Cited by-同舟云学术

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Relationship between CH₃OD Abundance and Temperature in the Orion KL Nebula

Published:2022-08-24 Issue:37 Volume:126 Page:6473-6482
ISSN:1089-5639
Container-title:The Journal of Physical Chemistry A
language:en
Short-container-title:J. Phys. Chem. A

Author:

Wilkins Olivia H.¹^ORCID,Blake Geoffrey A.¹²

Affiliation:

1. Division of Chemistry and Chemical Engineering, California Institute of Technology, Pasadena, California 91125, United States

2. Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, California 91125, United States

Funder

National Radio Astronomy Observatory

Division of Astronomical Sciences

Division of Graduate Education

National Aeronautics and Space Administration

Publisher

American Chemical Society (ACS)

Subject

Physical and Theoretical Chemistry

Link

https://pubs.acs.org/doi/pdf/10.1021/acs.jpca.2c01309

Reference60 articles.

1. 67P/Churyumov-Gerasimenko, a Jupiter family comet with a high D/H ratio

2. The primordial deuterium abundance at zabs = 2.504 from a high signal-to-noise spectrum of Q1009+2956

3. Deuteration and evolution in the massive star formation process

4. Complex Organic Interstellar Molecules

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1. CH₃OH and Its Deuterated Species in the Disk/Envelope System of the Low-mass Protostellar Source B335;The Astrophysical Journal;2024-07-01

2. Rotational spectroscopy of CH₃OD with a reanalysis of CH₃OD toward IRAS 16293–2422;Astronomy & Astrophysics;2024-07

3. Spectroscopic shifts in deuterated methanol induced by variation of me/mp;Physical Review A;2024-07-01

4. 10 Years of the ACS PHYS Astrochemistry Subdivision;The Journal of Physical Chemistry A;2022-09-29

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