Hostname: page-component-586b7cd67f-2plfb Total loading time: 0 Render date: 2024-11-23T02:20:27.565Z Has data issue: false hasContentIssue false

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
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

References

Brogan, C. L., Hunter, T. R., Cyganowski, C. J., Friesen, R., et al. 2011, ApJLGoogle Scholar
Brogan, C. L., Hunter, T. R., Cyganowski, C. J., Indebetouw, R., et al. 2009, ApJ, 707, 1CrossRefGoogle Scholar
Brogan, C. L., Hunter, T. R., Indebetouw, R., et al. 2008, Ap&SS, 313, 53Google Scholar
Brogan, C. L., Chandler, C. J., Hunter, T. R., et al. 2007, ApJ, 660, L133CrossRefGoogle Scholar
Churchwell, E. 2002, ARAA, 40, 27CrossRefGoogle Scholar
Cyganowski, C. J., Brogan, C. L., & Hunter, T. R. 2011, ApJ, 743, 56CrossRefGoogle Scholar
Cyganowski, C. J., Brogan, C. L., Hunter, T. R., & Churchwell, E. 2009, ApJ, 702, 1615CrossRefGoogle Scholar
Cyganowski, C. J., et al. 2008, AJ, 136, 2391CrossRefGoogle Scholar
Cyganowski, C. J., Brogan, C. L., & Hunter, T. R. 2007, AJ, 134, 346CrossRefGoogle Scholar
Devine, K., Chandler, C. J., Brogan, C. L., et al. 2011, ApJ, 733, 44Google Scholar
Ellingsen, S. P. et al. 2007, IAU Symposium, 242, 213CrossRefGoogle Scholar
Hunter, T. R., Brogan, C. L., Indebetouw, R., & Cyganowski, C. J. 2008, ApJ, 680, 1271CrossRefGoogle Scholar
Hunter, T. R., Brogan, C. L., Megeath, S., et al. 2006, ApJ, 649, 888CrossRefGoogle Scholar
Menten, K. M., Walmsley, C. M., Henkel, C., & Wilson, T. L. 1986, A&A, 157, 318Google Scholar
Molinari, S., Brand, J., Cesaroni, R., & Palla, F. 1996, A&A, 308, 573Google Scholar
Reid, M. J., et al. 2009, ApJ, 700, 137CrossRefGoogle Scholar
Rathborne, J. M., Jackson, J. M., & Simon, R. 2006, ApJ, 641, 389CrossRefGoogle Scholar
Rosolowsky, E., Dunham, M. K., Ginsburg, A., et al. 2010, ApJS, 188, 123CrossRefGoogle Scholar
Sridharan, T. K., Beuther, H., Schilke, P., Menten, K. M., & Wyrowski, F. 2002, ApJ, 566, 931CrossRefGoogle Scholar
Zhang, Q., Hunter, T. R., Sridharan, T. K., & Cesaroni, R. 1999, ApJ, 527, L117CrossRefGoogle Scholar
Zinnecker, H. & Yorke, H. W. 2007, ARAA, 45, 481CrossRefGoogle Scholar