CH+(1-0) and 13CH+(1-0) absorption lines in the direction of massive star-forming regions
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P. Hennebelle | K. Menten | M. Pérault | K. Klein | P. Encrenaz | C. Joblin | J. Goicoechea | F. Boulanger | M. Gerin | D. Teyssier | E. Dartois | T. Bell | J. Black | J. Stutzki | C. Vastel | J. Cernicharo | D. Lis | L. Samoska | C. Persson | E. Falgarone | A. Cros | R. Kołos | S. Schlemmer | P. Goldsmith | T. Phillips | T. Giesen | H. Gupta | E. Herbst | S. Lord | P. Morris | D. Neufeld | J. Pearson | R. Plume | M. Salez | J. Zmuidzinas | T. Geballe | M. Schmidt | R. Shipman | R. Monje | Shanshan Yu | P. Sonnentrucker | P. Planesas | L. Ravera | J. Martín-Pintado | R. Szczerba | A. Lorenzani | P. Hily-Blant | I. Péron | A. Coutens | S. Philipp | C. Gry | J. Krełowski | M. Luca | B. Mookerjea | B. Godard | M. Kaźmierczak | P. Cais | A. Tielens | P. Gaufre
[1] P. Hennebelle,et al. Interstellar CH absorption in the diffuse interstellar medium along the sight-lines to G10.6-0.4 (W31C), W49N, and W51 , 2010 .
[2] S. Bontemps,et al. Variations in H2O+/H2O ratios toward massive star-forming regions , 2010, 1007.4370.
[3] P. Hennebelle,et al. Detection of hydrogen fluoride absorption in diffuse molecular clouds with Herschel/HIFI: an ubiquitous tracer of molecular gas , 2010, 1007.2148.
[4] K. Menten,et al. Herschel/HIFI deepens the circumstellar NH3 enigma , 2010, 1007.1413.
[5] C. Kramer,et al. Strong CH+ J = 1–0 emission and absorption in DR21 , 2010, 1007.1420.
[6] M. Gerin,et al. Molecular absorption lines toward star-forming regions: a comparative study of HCO+, HNC, HCN, and CN , 2010, 1006.0582.
[7] S. Ott,et al. Herschel Space Observatory - An ESA facility for far-infrared and submillimetre astronomy , 2010, 1005.5331.
[8] S. J. Liu,et al. Herschel : the first science highlights Special feature L etter to the E ditor The Herschel-SPIRE instrument and its in-flight performance , 2010 .
[9] P. Hennebelle,et al. Strong absorption by interstellar hydrogen fluoride: Herschel/HIFI observations of the sight-line to G10.6-0.4 (W31C) , 2010, 1005.1671.
[10] J. Goicoechea,et al. THE CHEMISTRY OF VIBRATIONALLY EXCITED H2 IN THE INTERSTELLAR MEDIUM , 2010, 1003.1375.
[11] J. Pety,et al. Intermittency of interstellar turbulence: extreme velocity-shears and CO emission on milliparsec scale , 2009, 0910.1766.
[12] E. Falgarone,et al. Models of turbulent dissipation regions in the diffuse interstellar medium , 2009, 0901.3712.
[13] T. Weselak,et al. Relation between CH cation and neutral/molecular hydrogen (Research Note) , 2008 .
[14] O. Stahl,et al. Interstellar 12C/13C from CH+ absorption lines: Results from an extended survey , 2007, 0711.2365.
[15] P. Hennebelle,et al. Effects of turbulent diffusion on the chemistry of diffuse clouds , 2007, 0704.3149.
[16] B. Drouin,et al. Laboratory Measurement of the J = 1-0 Transition of CH+ , 2006 .
[17] A. Robin,et al. Modelling the Galactic Interstellar Extinction Distribution in Three Dimensions , 2005, astro-ph/0604427.
[18] E. Falgarone,et al. First Detection of 13CH+ (J = 1-0) , 2005 .
[19] C. Kramer,et al. The Herschel-Heterodyne Instrument for the Far-Infrared (HIFI) , 2005, Infrared and Millimeter Waves, Conference Digest of the 2004 Joint 29th International Conference on 2004 and 12th International Conference on Terahertz Electronics, 2004..
[20] G. P. Forêts,et al. C‐type shocks in the interstellar medium: profiles of CH+ and CH absorption lines , 1998 .
[21] M. Barlow,et al. Discovery of Far-Infrared Pure Rotational Transitions of CH+ in NGC 7027 , 1997 .
[22] D. Lambert,et al. A Very high resolution survey of interstellar CH and CH , 1995 .
[23] G. Herzberg,et al. Note on CH^{+} in Interstellar Space and in the Laboratory. , 1941 .