OH emission from warm and dense gas in the Orion Bar PDR-Reference-Cited by-同舟云学术

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OH emission from warm and dense gas in the Orion Bar PDR

Published:2011-05-25 Issue: Volume:530 Page:L16
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Goicoechea J. R.,Joblin C.,Contursi A.,Berné O.,Cernicharo J.,Gerin M.,Le Bourlot J.,Bergin E. A.,Bell T. A.,Röllig M.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361/201116977/pdf

Reference38 articles.

1. THE CHEMISTRY OF VIBRATIONALLY EXCITED H2IN THE INTERSTELLAR MEDIUM

2. H2Pure Rotational Lines in the Orion Bar

3. Kinetic temperatures in the Orion Bar

4. Herschelobservations of EXtra-Ordinary Sources (HEXOS): The present and future of spectral surveys withHerschel/HIFI

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1. PDRs4All;Astronomy & Astrophysics;2024-07

2. OH as a probe of the warm-water cycle in planet-forming disks;Nature Astronomy;2024-02-23

3. Effect of temperature on the gas-phase reaction of CH₃CN with OH radicals: experimental (T = 11.7–177.5 K) and computational (T = 10–400 K) kinetic study;Physical Chemistry Chemical Physics;2024

4. The Origin of Dust Polarization in the Orion Bar;The Astrophysical Journal;2023-07-01

5. OH mid-infrared emission as a diagnostic of H₂O UV photodissociation;Astronomy & Astrophysics;2023-03

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