arXivDaily arXiv每日学术速递 周一至周五更新
arXiv 0903.3210astro-ph.HE
收藏

SAX J1808 .4-3658:高分辨率光谱学和低能量下脉冲分数的降低

SAX J1808.4-3658: high resolution spectroscopy and decrease of pulsed fraction at low energies

Alessandro Patruno, Nanda Rea, Diego Altamirano, Manuel Linares, R. Wijnands, M. van der Klis

摘要:

XMM-牛顿在2008年爆发期间观测到了吸积毫秒脉冲星SAX J1808.4-3658。我们目前的时间和光谱分析,这一观察,特别是第一次脉冲轮廓研究低于2千电子伏,高分辨率的光谱分析,这个源在爆发。结合光谱和脉冲轮廓分析表明,存在一个强大的非脉冲源低于2千电子伏,大大减少了脉冲的分数和硬脉冲的组件,产生显着的双峰在较高的能量配置文件。我们还研究了SAXJ1808.4 -3658的高分辨光栅谱,发现了几条吸收边和氧吸收线,并据此以模型无关的方式推测了SAXJ1808.4 -3658方向上几种元素的星际柱密度。

英文摘要:

XMM-Newton observed the accreting millisecond pulsar SAX J1808.4-3658 during its 2008 outburst. We present timing and spectral analyses of this observation, in particular the first pulse profile study below 2 keV, and the high-resolution spectral analysis of this source during the outburst. Combined spectral and pulse profile analyses suggest the presence of a strong unpulsed source below 2 keV that strongly reduces the pulsed fraction and a hard pulsed component that generates markedly double peaked profiles at higher energies. We also studied the high-resolution grating spectrum of SAX J1808.4-3658, and found several absorption edges and Oxygen absorption lines with whom we infer, in a model independent way, the interstellar column densities of several elements in the direction of SAX J1808.4-3658.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

↑