First hard X-ray detection and broad-band X-ray study of the unidentified transient AX J1949.8+2534

被引:4
|
作者
Sguera, V. [1 ]
Sidoli, L. [2 ]
Paizis, A. [2 ]
Masetti, N. [1 ]
Bird, A. J. [3 ]
Bazzano, A. [4 ]
机构
[1] INAF, Ist Astrofis Spaziale & Fis Cosm, Via Gobeni 101, I-40129 Bologna, Italy
[2] INAF, Ist Astrofis Spaziale & Fis Cosm, Via E Rossini 15, I-20133 Milan, Italy
[3] Univ Southampton, Sch Phys & Astron, Univ Rd, Southampton SO17 1BJ, Hants, England
[4] INAF, Ist Astrofis & Planetol Spaziali, Via Fosso del Cavaliers 100, I-00133 Rome, Italy
关键词
X-rays: binaries; X-rays: individual: AX J1949.8-2534; CATACLYSMIC VARIABLES; SWIFT/XRT OBSERVATIONS; INTEGRAL/IBIS; DISCOVERY; BEHAVIOR; SAMPLE; IBIS;
D O I
10.1093/mnras/stx1111
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the results from INTEGRAL and Swift/XRT observations of the hitherto poorly studied unidentified X-ray transient AX J1949.8+2534, and on archival multiwavelength observations of field objects. Bright hard X-ray outbursts have been discovered above 20 keV for the first time, the measured duty cycle and dynamic range are of the order of similar to 4 per cent and >= 630, respectively. The source was also detected during a low soft X-ray state (similar to 2 x 10(-12) erg cm(-2)s(-1)) thanks to a Swift/XRT followup, which allowed for the first time to perform a soft X-ray spectral analysis as well as significantly improve the source positional uncertainty from arcminute to arcsecond size. From archival near-infrared data, we pinpointed two bright objects as most likely counterparts whose photometric properties are compatible with an early-type spectral nature. This strongly supports a high-mass X-ray binary (HMXB) scenario for AX J1949.8+2534, specifically a Supergiant Fast X-ray Transient (more likely) or alternatively a Be HMXB.
引用
收藏
页码:3901 / 3908
页数:8
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