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 H 2 O abundance

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[1] [1,Kristensen, L.E.
[2] 2,Van Dishoeck, E.F.
[3] Mottram, J.C.
[4] Karska, A.
[5] Ylldlz, U.A.
[6] Bergin, E.A.
[7] Bjerkeli, P.
[8] Cabrit, S.
[9] Doty, S.
[10] Evans, N.J.
[11] Gusdorf, A.
[12] Harsono, D.
[13] Herczeg, G.J.
[14] 14,Johnstone, D.
[15] Jørgensen, J.K.
[16] 2,Van Kempen, T.A.
[17] 17,Lee, J.-E.
[18] 19,Maret, S.
[19] Tafalla, M.
[20] Visser, R.
[21] Wampfler, S.F.
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| 1600年 / EDP Sciences卷 / 605期
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  • [1] 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.
    Yildiz, U. A.
    Bergin, E. A.
    Bjerkeli, P.
    Cabrit, S.
    Doty, S.
    Evans, N. J., II
    Gusdorf, A.
    Harsono, D.
    Herczeg, G. J.
    Johnstone, D.
    Jorgensen, J. K.
    van Kempen, T. A.
    Lee, J. -E.
    Maret, S.
    Tafalla, M.
    Visser, R.
    Wampfler, S. F.
    ASTRONOMY & ASTROPHYSICS, 2017, 605
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