CS J = 7 -> 6 Mapping of Massive Star Formation Regions Associated with Water Masers

Claudia Knez , Yancy L. Shirley , Neal J. Evans II , Kaisa E. Mueller (Department of Astronomy , The University of Texas at Austin)

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classification 🌌 astro-ph

keywords determineassociatedbeencarlocombiningcontinuumcorecores

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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.

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CS J = 7 -> 6 Mapping of Massive Star Formation Regions Associated with Water Masers

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