Methanol abundance in low mass protostars
| dc.creator | Maret, S. | |
| dc.date | 2004-11-12 | |
| dc.date.accessioned | 2026-07-07T02:15:48Z | |
| dc.date.available | 2026-07-07T02:15:48Z | |
| dc.description | Methanol lines observations of a sample of low mass Class 0 protostars are presented. Using a 1D radiative transfer model, I show that several protostars have large abundance jumps in the inner hot and dense region of envelopes, probably because of thermal grain mantle evaporation. These abundances are compared with a grain surface chemistry model. | |
| dc.description | 2 pages, 2 figures, Proceeding of the conference "The dusty and molecular universe", 27-29 October 2004, Paris, France | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0411350 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0411350 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/8547 | |
| dc.subject | Astrophysics | |
| dc.title | Methanol abundance in low mass protostars | |
| dc.type | text |