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

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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.;
  • Publisher: EDP SCIENCES S A
  • Journal: ASTRONOMY & ASTROPHYSICS (issn: 0004-6361)
  • Publisher copyright policies & self-archiving
  • Related identifiers: doi: 10.1051/0004-6361/201321954
  • Subject: Astrophysics - Solar and Stellar Astrophysics | ISM: jets and outflows | [ SDU.ASTR.SR ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR] | stars: protostars | [SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR] | [ PHYS.ASTR.SR ] Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR] | molecular processes | infrared: ISM | astrochemistry | [PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]

Aims: Our aim is to study the response of the gas-to-energetic processes associated with high-mass star formation and compare it with previously published studies on low- and intermediate-mass young stellar objects (YSOs) using the same methods. The quantified far-IR li... View more
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