The γ-ray pulsar J1932+1916 in X-rays

被引：0

作者：

Karpova, A. ^{[1
]}

Shternin, P. ^{[1
]}

Zyuzin, D. ^{[1
]}

Danilenko, A. ^{[1
]}

Shibanov, Yu ^{[1
]}

机构：

[1] Ioffe Inst, Politekhnicheskaya 26, St Petersburg 194021, Russia

来源：

INTERNATIONAL CONFERENCE PHYSICA.SPB/2016 | 2017年 / 929卷

关键词：

D O I：

10.1088/1742-6596/929/1/012011

中图分类号：

O59 [应用物理学];

学科分类号：

摘要：

We report the results of a simultaneous analysis of the archival Suzaku and Swift X-ray data of the gamma-ray pulsar J1932+1916 field. A point-like source and diffuse emission around it were detected at the gamma-ray position of the pulsar. Their spectral properties allow one to suggest that Suzaku and Swift detected the X-ray counterpart of PSR J1932+1916. Using of the interstellar absorption-distance relations, we constrain the distance to the pulsar in the range of 2-6 kpc. We also discuss a possible association of the pulsar with the supernova remnant G54.4-0.3.

引用

页数：4

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