OH as an Alternate Tracer for Molecular Gas: Excitation Temperatures of the OH 18 cm Main Lines in W5
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/858/i=1/a=57/pdf
Reference29 articles.
1. THE STRUCTURE OF DARK MOLECULAR GAS IN THE GALAXY. I. A PILOT SURVEY FOR 18 cm OH EMISSION TOWARDl≈ 105°,b≈ +1°
2. FAINT EXTENDED OH EMISSION FROM THE LOCAL INTERSTELLAR MEDIUM IN THE DIRECTIONl≈ 108°,b≈ 5°
3. ERRATUM: “FAINT EXTENDED OH EMISSION FROM THE LOCAL INTERSTELLAR MEDIUM IN THE DIRECTION l ≈ 108°, b ≈ 5°” (2012, AJ, 143, 97)
4. The NRAO VLA Sky Survey
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2. GNOMES II: Analysis of the Galactic diffuse molecular ISM in all four ground state hydroxyl transitions using Amoeba;Publications of the Astronomical Society of Australia;2023
3. HyGAL: Characterizing the Galactic Interstellar Medium with Observations of Hydrides and Other Small Molecules. I. Survey Description and a First Look Toward W3(OH), W3 IRS5, and NGC 7538 IRS1;The Astrophysical Journal;2022-05-01
4. SPLASH: the Southern Parkes Large-Area Survey in Hydroxyl – data description and release;Monthly Notices of the Royal Astronomical Society;2022-03-14
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