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VLA Detections of Stellar Winds Arising from the Galactic Center Arches Cluster

Published online by Cambridge University Press:  13 May 2016

Cornelia C. Lang ,
W.M. Goss  and
L.F. Rodríguez
Cornelia C. Lang
Affiliation:
University of Massachusetts, Amherst, MA 01003, USA
W.M. Goss
Affiliation:
National Radio Astronomy Observatory, Socorro, NM 87801, USA
L.F. Rodríguez
Affiliation:
Instituto de Astronomía, UNAM, Morelia, Michoacán 58089, México

Abstract

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VLA detections have been made of 8 sources in the Galactic center Arches cluster. All sources have spectra consistent with those expected for stellar wind emission. Positional correspondence between these sources and near-infrared detections of mass-losing stars confirms that we are detecting stellar wind emission from Arches cluster members.

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. 276 - 279
Copyright
Copyright © Astronomical Society of the Pacific 2001 

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