The Bulletin of The Korean Astronomical Society (천문학회보)
- Volume 40 Issue 2
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- Pages.52.3-53
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- 2015
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- 1226-2692(pISSN)
HCO+ Observations toward Compact Radio Continuum Sources Using the KVN 21-m Telescopes to Trace Dark Molecular Gas
- Park, Geumsook (Seoul National University) ;
- Koo, Bon-Chul (Seoul National University) ;
- Kim, Kee-Tae (Korea Astronomy and Space Science Institute) ;
- Byun, Do-Young (Korea Astronomy and Space Science Institute) ;
- Heiles, Carl (UC Berkeley)
- Published : 2015.10.15
Abstract
It has been known that there is "dark gas" invisible either in 21-cm HI or 2.6-mm CO emission which are general tracers of atomic and molecular gas, respectively. Many researchers consider that the dark gas is "Dark Molecular Gas (DMG)" composed of CO-free
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