SO survey of massive cores
Abstract
We present the results of a survey of several tens of dense high mass star forming (HMSF) cores in three transitions of the SO molecule at 30 and 100 GHz with the 100-m Effelsberg and 20-m Onsala radio telescopes. The physical parameters of the cores are estimated from the line ratios and column densities. Relative abundances are derived as well.
- Publication:
-
Astrochemistry VII: Through the Cosmos from Galaxies to Planets
- Pub Date:
- September 2018
- DOI:
- arXiv:
- arXiv:1711.09380
- Bibcode:
- 2018IAUS..332..274Z
- Keywords:
-
- ISM: clouds;
- ISM: molecules;
- ISM: abundances;
- Astrophysics - Astrophysics of Galaxies
- E-Print:
- 5 pages, 4 figues, to be published in Proceedings of the IAU Symposium No. 332 "Astrochemistry VII - Through the Cosmos from Galaxies to Planets"