New insights on the HCl abundance in the interstellar medium | Zendy

Mathieu Lanza | Zendy; Yulia N. Kalugina | Zendy; L. Wiesenfeld | Zendy; Alexandre Faure | Zendy; François Lique | Zendy

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New insights on the HCl abundance in the interstellar medium

Author(s) -

Mathieu Lanza,

Yulia N. Kalugina,

L. Wiesenfeld,

Alexandre Faure,

François Lique

Publication year - 2014

Publication title -

monthly notices of the royal astronomical society

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 2.058

H-Index - 383

eISSN - 1365-8711

pISSN - 0035-8711

DOI - 10.1093/mnras/stu1371

Subject(s) - chlorine , physics , interstellar medium , excitation , abundance (ecology) , line (geometry) , reaction rate , atomic physics , astrophysics , chemistry , quantum mechanics , galaxy , fishery , biology , biochemistry , geometry , mathematics , organic chemistry , catalysis

HCl is supposed to be one of the main chlorine carriers in the interstellar medium (ISM). Then, accurate knowledge of chlorine chemistry requires accurate estimating the HCl abundance in molecular clouds which in turn requires the calculation of collisional excitation rate coefficients for the HCl molecule due to collisions with the most abundant collisional partner in the ISM. In this paper, we r...

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