New rate coefficients of CS in collision with para- and ortho-H2 and astrophysical implications
dc.creator | Denis-Alpizar O. | |
dc.creator | Stoecklin T. | |
dc.creator | Guilloteau S. | |
dc.creator | Dutrey A. | |
dc.date.accessioned | 2020-09-02T22:16:16Z | |
dc.date.accessioned | 2022-11-08T20:27:07Z | |
dc.date.available | 2020-09-02T22:16:16Z | |
dc.date.available | 2022-11-08T20:27:07Z | |
dc.date.created | 2020-09-02T22:16:16Z | |
dc.date.issued | 2018 | |
dc.identifier | 478, 2, 1811-1817 | |
dc.identifier | 00358711 | |
dc.identifier | https://hdl.handle.net/20.500.12728/4262 | |
dc.identifier.uri | https://repositorioslatinoamericanos.uchile.cl/handle/2250/5146329 | |
dc.language | en | |
dc.publisher | Oxford University Press | |
dc.subject | Astrochemistry | |
dc.subject | ISM: molecules | |
dc.subject | Molecular data | |
dc.subject | Molecular processes | |
dc.subject | Scattering | |
dc.title | New rate coefficients of CS in collision with para- and ortho-H2 and astrophysical implications | |
dc.type | Article |