SO survey of massive cores
arXiv:1711.09380 · doi:10.1017/S1743921317007694
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.
5 pages, 4 figues, to be published in Proceedings of the IAU Symposium No. 332 "Astrochemistry VII - Through the Cosmos from Galaxies to Planets"