Origin of warm and hot gas emission from low-mass protostars: Herschel-HIFI 
observations of CO J = 16–15 - I. Line profiles, physical conditions, and H2O 
abundance

Kristensen, L. E.; Van Dishoeck, E. F.; Mottram, J. C.; Karska, A.; Yıldız, U. A.; Bergin, E. A.; Bjerkeli, P.; Cabrit, S.; Doty, S.; Evans, N. J. II; Gusdorf, A.; Harsono, D.; Herczeg, G. J.; Johnstone, D.; Jørgensen, J. K.; van Kempen, T. A.; Lee, J.-E.; Maret, S.; Tafalla, M.; Visser, R.; Wampfler, S. F.

doi:10.1051/0004-6361/201630127

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Origin of warm and hot gas emission from low-mass protostars: Herschel-HIFI observations of CO J = 16–15 - I. Line profiles, physical conditions, and H2O abundance

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Van Dishoeck, E. F.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Kristensen, L. E., Van Dishoeck, E. F., Mottram, J. C., Karska, A., Yıldız, U. A., Bergin, E. A., et al. (2017). Origin of warm and hot gas emission from low-mass protostars: Herschel-HIFI observations of CO J = 16–15 - I. Line profiles, physical conditions, and H2O abundance. Astronomy & Astrophysics, 605: A93. doi:10.1051/0004-6361/201630127.

Cite as: https://hdl.handle.net/11858/00-001M-0000-002E-5202-E

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