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High-mass Star Formation in the Regions IRAS 19217+1651 and 23151+5912

Published online by Cambridge University Press:  24 July 2012

V. Migenes ,
I. T. Rodríguez  and
M. A. Trinidad
V. Migenes
Affiliation:
Brigham Young University, Department of Physics and Astronomy ESC-N145, Provo, UT. 84602USA email: [email protected]
I. T. Rodríguez
Affiliation:
University of Guanajuato, Department of Astronomy, Aptd. Postal 144 Guanajuato, GTO. 36000Mexico email: [email protected], [email protected]
M. A. Trinidad
Affiliation:
University of Guanajuato, Department of Astronomy, Aptd. Postal 144 Guanajuato, GTO. 36000Mexico email: [email protected], [email protected]
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Abstract

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We present and discuss VLA-EVLA high-sensitivity and spatial resolution observations of Water Vapor MASERs and continuum emission towards two sources that have been proposed in the literature to be high-mass star forming regions: IRAS 19217+1651 and 23151+5912. Our results indicate the presence of disks which can confirm that these regions are high-mass star forming regions.

Keywords

stars: formationstars: high massISM: HII regionsmasers
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S287: Cosmic Masers - from OH to H0 , January 2012 , pp. 182 - 183
Copyright
Copyright © International Astronomical Union 2012

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