A self-consistent approach to the reflection component in 4U 1705-44

被引：0

作者：

D'Ai, A. ^{[1
]}

Di Salvo, T. ^{[1
]}

Iaria, R. ^{[1
]}

Papitto, A. ^{[2
]}

Ballantyne, D. ^{[3
]}

机构：

[1] Univ Palermo, DSFA, Via Archirafi 36, I-90123 Palermo, Italy

[2] Univ Cagliari, Dipartimento Fis, I-09042 Monserrato, Italy

[3] Ctr Relativist Astrophys, Georgia Tech, MA USA

来源：

X-RAY ASTRONOMY-2009: PRESENT STATUS, MULTI-WAVELENGTH APPROACH AND FUTURE PERSPECTIVES, PROCEEDINGS | 2010年 / 1248卷

关键词：

accretion discs; stars: individual: 4U 1705-44; stars: neutron stars; X-ray: stars; X-ray: spectrum; X-ray: general; DISK;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

High-resolution spectroscopy has recently revealed in many neutron-star Low-Mass Xray binaries that the shape of the broad iron line observed in the 6.4-6.97 keV range is consistently well fitted by a relativistically smeared line profile. We show here spectral fitting results using a newly developed self-consistent reflection model on XMM-Newton data of the LMXB 4U 1705-44 during a period when the source was in a bright soft state. This reflection model adopts a blackbody prescription for the shape of the impinging radiation field, that we physically associate with the boundary layer emission.

引用

页码：63 / +

页数：2

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