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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
Affiliation:
Brigham Young University, Department of Physics and Astronomy ESC-N145, Provo, UT. 84602USA email: vmigenes@byu.edu
I. T. Rodríguez
Affiliation:
University of Guanajuato, Department of Astronomy, Aptd. Postal 144 Guanajuato, GTO. 36000Mexico email: tatiana@astro.ugto.mx, trinidad@astro.ugto.mx
M. A. Trinidad
Affiliation:
University of Guanajuato, Department of Astronomy, Aptd. Postal 144 Guanajuato, GTO. 36000Mexico email: tatiana@astro.ugto.mx, trinidad@astro.ugto.mx
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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.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2012

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