X-RAY AND RADIO OBSERVATIONS OF THE MASSIVE STAR-FORMING REGION IRAS 20126+4104

被引:7
|
作者
Montes, V. A. [1 ]
Hofner, P. [1 ]
Anderson, C. [1 ,2 ]
Rosero, V. [1 ,2 ]
机构
[1] New Mexico Inst Min & Technol, Dept Phys, Socorro, NM 87801 USA
[2] Natl Radio Astron Observ, Socorro, NM 87801 USA
来源
关键词
open clusters and associations: individual (IRAS 20126+4104); radio continuum: stars; stars: formation; stars: pre-main sequence; X-rays: stars; YOUNG STARS; DISK; IRAS-20126+4104; ACCRETION; OUTFLOW; SYSTEM; RESOLUTION; CLUSTERS; CHANDRA;
D O I
10.1088/0067-0049/219/2/41
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present results from Chandra ACIS-I and Karl G. Jansky Very Large Array 6 cm continuum observations of the IRAS 20126+4104 massive star-forming region. We detect 150 X-ray sources within the 17' x 17' ACIS-I field, and a total of 13 radio sources within the 9'.2 primary beam at 4.9 GHz. Among these observtions are the first 6 cm detections of the central sources reported by Hofner et al., namely,. I20N1, I20S, and I20var. A new variable radio source is also reported. Searching the 2MASS archive, we identified 88 near-infrared (NIR) counterparts to the X-ray sources. Only four of the X-ray sources had 6 cm counterparts. Based on an NIR color-color analysis and on the Besancon simulation of Galactic stellar populations, we estimate that approximately 80 X-ray sources are associated with this massive star-forming region. We detect an increasing surface density of X-ray sources toward the massive protostar and infer the presence of a cluster of at least 43 young stellar objects within a distance of 1.2 pc from the massive protostar.
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页数:15
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