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Early results from a diagnostic 1.3 cm survey of massive young protostars

Published online by Cambridge University Press:  24 July 2012

Crystal L. Brogan
Affiliation:
National Radio Astronomy Observatory (NRAO), 520 Edgemont Rd, Charlottesville, VA 22903, USA email: [email protected]
Todd R. Hunter
Affiliation:
National Radio Astronomy Observatory (NRAO), 520 Edgemont Rd, Charlottesville, VA 22903, USA email: [email protected]
Claudia J. Cyganowski
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138, USA
Remy Indebetouw
Affiliation:
National Radio Astronomy Observatory (NRAO), 520 Edgemont Rd, Charlottesville, VA 22903, USA email: [email protected] University of Virginia, Charlottesville, VA 22903, USA
Rachel Friesen
Affiliation:
National Radio Astronomy Observatory (NRAO), 520 Edgemont Rd, Charlottesville, VA 22903, USA email: [email protected]
Claire Chandler
Affiliation:
National Radio Astronomy Observatory (NRAO), Socorro, New Mexico, 87801, 8USA
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Abstract

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We have used the recently-upgraded Karl G. Jansky Very Large Array (JVLA) to conduct a K-band (~24 GHz) study of 22 massive young stellar objects in 1.3 cm continuum and a comprehensive set of diagnostic lines. This survey is unique in that it samples a wide range of massive star formation signposts simultaneously for the first time. In this proceeding we present preliminary results for the 11 sources in the 2-4 kpc distance bin. We detect compact NH3 cores in all of the fields, with many showing emission up through the (6,6) transition. Maser emission in the 25 GHz CH3OH ladder is present in 7 of 11 sources. We also detect non-thermal emission in the NH3 (3,3) transition in 7 of 11 sources.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2012

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