Sample of optically unidentified X-ray binaries in the Galactic bulge: constraints on the physical nature from infrared photometric surveys

被引：5
|
作者：
Zolotukhin, Ivan Yu [1 ,2 ]
Revnivtsev, Mikhail G. [3 ]
机构：
[1] IRAP, CNRS, 9 Ave Colonel Roche,BP 44346, F-31028 Toulouse 4, France
[2] Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow 119992, Russia
[3] Russian Acad Sci, Space Res Inst, Moscow 117997, Russia
来源：
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2015年 / 446卷 / 03期
基金：
美国国家航空航天局; 俄罗斯基础研究基金会;
关键词：
X-rays: binaries; X-rays: individual: AX J1754.2-2754; X-rays: individual: IGR J17464-2811; X-rays: individual: IGR J17597-2201; X-rays: individual: Ser X-1; infrared; SPECTRAL ENERGY-DISTRIBUTIONS; DISC INSTABILITY MODEL; LUMINOSITY FUNCTION; SKY SURVEY; INTERSTELLAR EXTINCTION; CHANDRA LOCALIZATIONS; INTEGRAL SOURCES; MILKY-WAY; PERSISTENT; CATALOG;
D O I：
10.1093/mnras/stu2212
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We report on archival near-infrared and mid-infrared observations of seven persistent Xray sources situated in the Galactic bulge, using data from the UK Infrared Telescope (UKIRT) Infrared Deep Sky Survey (UKIDSS), the Spitzer Galactic Legacy Infrared Mid-Plane Survey Extraordinaire (GLIMPSE) and the Wide-field Infrared Survey Explorer (WISE) all-sky survey. We were able to successfully identify or provide upper flux limits for the systems SAX J1747.0-2853, IGR J17464-2811, AX J1754.2-2754, IGR J17597-2201, IGR J18134-1636, IGR J18256-1035 and Ser X-1 and constrain the nature of these systems. In the case of IGR J17597-2201, we present arguments that the source accretes matter from the stellar wind rather than via Roche-lobe overflow of the secondary. We suggest that, at its X-ray luminosity of 10(34) 3 5 erg s(1), we are probing the poorly known class of wind-fed low-mass X-ray binaries (LMXBs).
引用
收藏
页码：2418 / 2427
页数：10
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