Hard spectra of X-ray pulsars from INTEGRAL data

被引:74
作者
Filippova, EV
Tsygankov, SS
Lutovinov, AA
Sunyaev, RA
机构
[1] Russian Acad Sci, Inst Space Res, Moscow 117810, Russia
[2] Max Planck Inst Astrophys, D-85741 Garching, Germany
来源
ASTRONOMY LETTERS-A JOURNAL OF ASTRONOMY AND SPACE ASTROPHYSICS | 2005年 / 31卷 / 11期
基金
俄罗斯基础研究基金会;
关键词
X-ray pulsars; neutron stars; spectra;
D O I
10.1134/1.2123288
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present spectra for 34 accretion-powers X-ray pulsars and one millisecond pulsar that were within the field of view of the INTEGRAL observatory over two years (December 2002-January 2005) of its in-orbit operation and that were detected by its instruments at a statistically significant level (> 8 sigma in the energy range 18-60 keV). There are seven recently discovered objects of this class among the pulsars studied: 2RXP J130159.6-635806, IGR/AX J16320-4751, IGR J16358-4726, AX J163904-4642, IGR J16465-4507, SAX/IGR J18027-2017, and AX J1841.0-0535. We have also obtained hard Xray (> 20 keV) spectra for the accretion-powered pulsars RX J0146.9+6121, AX J1820.5-1434, and AX J1841.0-0535 for the first time. We analyze the evolution of spectral parameters as a function of the intensity of the sources and compare these with the results of previous studies. (c) 2005 Pleiades Publishing, Inc.
引用
收藏
页码:729 / 747
页数:19
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