OH 18 cm observations of the intermediate-velocity molecular cloud G211+63-Reference-Cited by-同舟云学术

OH 18 cm observations of the intermediate-velocity molecular cloud G211+63

Published:2018-07-18 Issue:3 Volume:480 Page:3503-3510
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Smith Allison J¹,Magnani Loris¹,Gonzalez Louis²,Robishaw Timothy³

Affiliation:

1. Department of Physics and Astronomy, University of Georgia, Athens, GA 30602, USA

2. Department of Physics and Astronomy, Georgia State University, Atlanta, GA 30302, USA

3. National Research Council Canada, Herzberg Astronomy and Astrophysics Programs, Dominion Radio Astrophysical Observatory, Penticton, BC V2A 6J9, Canada

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/480/3/3503/25519286/sty1887.pdf

Reference44 articles.

1. FAINT EXTENDED OH EMISSION FROM THE LOCAL INTERSTELLAR MEDIUM IN THE DIRECTIONl≈ 108°,b≈ 5°

2. THE STRUCTURE OF DARK MOLECULAR GAS IN THE GALAXY. I. A PILOT SURVEY FOR 18 cm OH EMISSION TOWARDl≈ 105°,b≈ +1°

3. Multiwavelength observations of cirrus clouds in the North Celestial Loop: a study of the OH emission

4. Multiwavelength observations of cirrus clouds in the North Celestial Loop: the transition from atomic to molecular gas

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1. Limits on the OH Molecule in the Smith High-velocity Cloud;The Astrophysical Journal;2024-04-26

2. A Search for OH 18 cm Emission from Intermediate-velocity Gas at High Galactic Latitudes;The Astrophysical Journal;2023-05-01