XMM-Newton spectral and timing observations of the millisecond pulsar PSR J0218+4232

被引：37

作者：

Webb, NA ^{[1
]}

Olive, JF ^{[1
]}

Barret, D ^{[1
]}

机构：

[1] UPS, CNRS, Ctr Etud Spatiale Rayonnements, F-31028 Toulouse 04, France

来源：

ASTRONOMY & ASTROPHYSICS | 2004年 / 417卷 / 01期

关键词：

X-rays : stars; stars : pulsars : individual : PSR J0218+4232; radiation mechanisms : non-thermal radiation mechanisms : thermal;

D O I：

10.1051/0004-6361:20040032

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present XMM-Newton MOS imaging and PN timing data of the millisecond pulsar PSR J0218+4232. We confirm the previously detected pulsations of PSR J0218+4232 and we show that the folded lightcurve is dependent on energy. We present the broad band (0.2-10.0 keV) spectrum of this millisecond pulsar, as well as the spectra of: the pulsed emission, the individual pulses, the interpulse and the non-pulsed region and we compare our results with previous data from Rosat, BeppoSAX and Chandra. We discuss the results of the spectral fitting in the context of recent pulsar models.

引用

页码：181 / 188

页数：8

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