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High Resolution Radio Continuum Observations of High Mass Star Formation Regions

Published online by Cambridge University Press:  13 May 2016

S. Kurtz ,
P. Hofner ,
C. Vargas  and
W. Díaz-Merced
S. Kurtz
Affiliation:
Universidad Nacional Autónoma de México Apdo. Postal 3-72 Xangari, C.P. 58089 Morelia, Mich. Mexico
P. Hofner
Affiliation:
University of Puerto Rico, Río Piedras P. 0. Box 23343, Rio Piedras PR 00931-3343 USA
C. Vargas
Affiliation:
University of Puerto Rico, Río Piedras P. 0. Box 23343, Rio Piedras PR 00931-3343 USA
W. Díaz-Merced
Affiliation:
University of Puerto Rico, Río Piedras P. 0. Box 23343, Rio Piedras PR 00931-3343 USA

Abstract

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We present high angular resolution centimeter and millimeter continuum observations of several galactic massive star formation regions. Using calibration techniques pioneered at the Very Large Array, we are able to obtain high quality images even under adverse conditions of phase stability. Techniques such as these will be essential if future millimeter arrays are to obtain high quality and high precision images. We provide a current summary of our on-going survey, and present images and a brief discussion of several of the more intriguing sources.

Type
Star Formation Regions and Outflow Processes in our Galaxy
Information
Symposium - International Astronomical Union , Volume 205: Galaxies and their Constituents at the Highest Angular Resolutions , 2001 , pp. 280 - 281
Copyright
Copyright © Astronomical Society of the Pacific 2001