pith. sign in

arxiv: 1711.09380 · v1 · pith:SM5EAP7Snew · submitted 2017-11-26 · 🌌 astro-ph.GA

SO survey of massive cores

classification 🌌 astro-ph.GA
keywords coressurveyabundancescolumndensedensitiesderivedeffelsberg
0
0 comments X
read the original 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.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.