Chandra imaging of the gamma-ray source GeV J1809-2327

被引：18
作者：
Braje, TM
Romani, RW
Roberts, MSE
Kawai, N
机构：
[1] Stanford Univ, Dept Phys, Stanford, CA 94305 USA
[2] McGill Univ, Dept Phys, Montreal, PQ H3A 2T8, Canada
[3] Tokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, Japan
[4] RIKEN, Wako, Saitama 3510198, Japan
来源：
ASTROPHYSICAL JOURNAL | 2002年 / 565卷 / 02期
关键词：
gamma rays : observations; pulsars : general; supernova remnants;
D O I：
10.1086/339419
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We report on Chandra imaging observations of the Galactic unidentified gamma-ray source GeV J1809-2327, comparing the X-ray images with new VLA 1.46 and 4.86 GHz maps. The X-ray images reveal a point source connected to a nonthermal X-ray/radio nebula, supporting a pulsar/wind model for the gamma-ray emitter. We also detect numerous X-ray sources from the young stellar association in the adjacent H II region S32.
引用
收藏
页码：L91 / L95
页数：5
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