The ortho-to-para ratio of H2Cl+: Quasi-classical trajectory calculations and new simulations in light of new observations
Artikel i vetenskaplig tidskrift, 2017
astrochemistry / ISM: molecules / quasars: individual: PKS 1830 / 211 / galaxies: ISM / quasars: absorption lines / radio lines: galaxies
Författare
R. Le Gal
University of Virginia
Harvard-Smithsonian Center for Astrophysics
C. Xie
University of New Mexico
E Herbst
University of Virginia
D. Talbi
Laboratoire Univers et Particules de Montpellier
H. Guo
University of New Mexico
Sebastien Muller
Chalmers, Rymd- och geovetenskap, Onsala rymdobservatorium
Astronomy and Astrophysics
0004-6361 (ISSN) 1432-0746 (eISSN)
Vol. 608 A96- A96Ämneskategorier
Astronomi, astrofysik och kosmologi
Fundament
Grundläggande vetenskaper
Infrastruktur
Onsala rymdobservatorium
DOI
10.1051/0004-6361/201731566