| Download | - View final version: Where is OH and does it trace the dark molecular gas (DMG)? (PDF, 2.0 MiB)
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| DOI | Resolve DOI: https://doi.org/10.3847/1538-4365/aaa762 |
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| Author | Search for: Li, Di; Search for: Tang, Ningyu; Search for: Nguyen, Hiep; Search for: Dawson, J. R.; Search for: Heiles, Carl; Search for: Xu, Duo; Search for: Pan, Zhichen; Search for: Goldsmith, Paul F.; Search for: Gibson, Steven J.; Search for: Murray, Claire E.; Search for: Robishaw, Tim1; Search for: Mcclure-Griffiths, N. M.; Search for: Dickey, John; Search for: Pineda, Jorge; Search for: Stanimirović, Snežana; Search for: Bronfman, L.; Search for: Troland, Thomas |
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| Affiliation | - National Research Council of Canada. Herzberg Astronomy and Astrophysics
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| Format | Text, Article |
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| Abstract | Hydroxyl (OH) is expected to be abundant in diffuse interstellar molecular gas because it forms along with H2 under similar conditions and forms within a similar extinction range. We have analyzed absorption measurements of OH at 1665 MHz and 1667 MHz toward 44 extragalactic continuum sources, together with the J = 1–0 transitions of 12CO, 13CO, and C18O, and the J = 2–1 transition of 12CO... |
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| Publication date | 2018-02-16 |
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| Publisher | American Astronomical Society |
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| In | |
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| Language | English |
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| Peer reviewed | Yes |
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| NPARC number | 23004142 |
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| Export citation | Export as RIS |
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| Report a correction | Report a correction (opens in a new tab) |
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| Record identifier | 9deb0e83-ec17-47de-b69a-fe4fce507710 |
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| Record created | 2018-10-02 |
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| Record modified | 2020-05-30 |
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