Far-infrared molecular lines from low- to high-mass star forming regions observed with Herschel

Article, Preprint OPEN
Karska, A.; Herpin, F.; Bruderer, S.; Goicoechea, J.; Herczeg, G.; Dishoeck, van, E.F.; San, José-García I.; Contursi, A.; Feuchtgruber, H.; Fedele, D.; Baudry, A.; Braine, J.; Chavarría, L.; Cernicharo, J.; Tak, F.; Wyrowski, F.; (2014)
  • Publisher: EDP SCIENCES S A
  • Journal: ASTRONOMY & ASTROPHYSICS (issn: 0004-6361)
  • Related identifiers: doi: 10.1051/0004-6361/201321954
  • Subject: Astrophysics - Solar and Stellar Astrophysics

(Abridged) We study the response of the gas to energetic processes associated with high-mass star formation and compare it with studies on low- and intermediate-mass young stellar objects (YSOs) using the same methods. The far-IR line emission and absorption of CO, H$_2... View more
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