Is there a cluster in the massive star forming region IRAS 20126+4104?

A Chandra X-ray Observatory ACIS-I observation and a 6 cm continuum radio observation with the Karl G. Jansky Very Large Array (VLA) together with a multiwavelength study in infrared (2MASS and Spitzer) and optical (USNO-B1.0) shows an increasing surface density of X-ray sources toward the massive p...

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Bibliographic Details
Published in:Proceedings of the International Astronomical Union 2015-08, Vol.12 (S316), p.157-158
Main Authors: Montes, V. A., Hofner, Peter, Anderson, C., Rosero, V.
Format: Article
Language:English
Subjects:
Astrophysics
Contributed Papers
Infrared imaging systems
Radio astronomy
Star & galaxy formation
Stars & galaxies
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Summary:A Chandra X-ray Observatory ACIS-I observation and a 6 cm continuum radio observation with the Karl G. Jansky Very Large Array (VLA) together with a multiwavelength study in infrared (2MASS and Spitzer) and optical (USNO-B1.0) shows an increasing surface density of X-ray sources toward the massive protostar. There are at least 43 YSOs within 1.2 pc distance from the massive protostar. This number is consistent with typical B-type stars clusters (Lada & Lada 2003).
ISSN:1743-9213
1743-9221
DOI:10.1017/S1743921315010558