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

页码：L91 / L95

页数：5

共 14 条

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