CS J = 7 -> 6 Mapping of Massive Star Formation Regions Associated with Water Masers
arXiv:astro-ph/0111105
Abstract
Twenty-four cores have been mapped in CS J = 7 -> 6 at the CSO. From the spectra we determine core sizes and virial masses. Combining results from the CS and dust continuum studies for M8E, we use Monte Carlo simulations for the CS emission to determine radial profiles.
2 pages to appear in Hot Star Workshop III: The Earliest Phases of Massive Star Birth, ASP Conference Series, 2002, ed. P.A. Crowther