The ortho-to-para ratio of H2Cl+: Quasi-classical trajectory calculations and new simulations in light of new observations
Journal article, 2017
astrochemistry / ISM: molecules / quasars: individual: PKS 1830 / 211 / galaxies: ISM / quasars: absorption lines / radio lines: galaxies
Author
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, Earth and Space Sciences, Onsala Space Observatory
Astronomy and Astrophysics
0004-6361 (ISSN) 1432-0746 (eISSN)
Vol. 608 A96- A96Subject Categories
Astronomy, Astrophysics and Cosmology
Roots
Basic sciences
Infrastructure
Onsala Space Observatory
DOI
10.1051/0004-6361/201731566