X-ray spectropolarimetry of the bright atoll Serpens X-1

被引:2
|
作者
Ursini, F. [1 ]
Gnarini, A. [1 ]
Bianchi, S. [1 ]
Bobrikova, A. [2 ]
Capitanio, F. [3 ]
Cocchi, M. [4 ]
Fabiani, S. [3 ]
Farinelli, R. [5 ]
Kaaret, P. [6 ]
Matt, G. [1 ]
Ng, M. [7 ]
Poutanen, J. [2 ]
Ravi, S. [7 ]
Tarana, A. [3 ]
机构
[1] Univ Roma Tre, Dipartimento Matemat & Fis, Via Vasca Navale 84, I-00146 Rome, Italy
[2] Univ Turku, Dept Phys & Astron, FI-20014 Turku, Finland
[3] INAF Ist Astrofis & Planetol Spaziali, Via Fosso Cavaliere 100, I-00133 Rome, Italy
[4] INAF Osservatorio Astron Cagliari, Via Sci 5, I-09047 Selargius, CA, Italy
[5] INAF Osservatorio Astrofis & Sci Spazio Bologna, Via P Gobetti 101, I-40129 Bologna, Italy
[6] NASA Marshall Space Flight Ctr, Huntsville, AL 35812 USA
[7] MIT, MIT Kavli Inst Astrophys & Space Res, Cambridge, MA 02139 USA
基金
芬兰科学院;
关键词
polarization; stars: neutron; X-rays: binaries; X-rays: individuals: Ser X-1; NEUTRON-STAR SURFACE; POLARIZATION PROPERTIES; GX 9+9; REFLECTION; SPECTRA; IXPE; POLARIMETRY; BURST; CONSTRAINTS; RADIATION;
D O I
10.1051/0004-6361/202451584
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present simultaneous X-ray polarimetric and spectral observations of the bright atoll source Ser X-1 carried out with the Imaging X-ray Polarimetry Explorer (IXPE), NICER, and NuSTAR. We obtain an upper limit of 2% (99% confidence level) on the polarization degree in the 2-8 keV energy band. We detect four type-I X-ray bursts, two of which during the IXPE observation. This is the first time that has IXPE observed type-I X-ray bursts, and it allows us to place an upper limit on their polarization degree; however, due to the limited total number of counts in each burst, we obtain a relatively high upper limit (80%). We confirm the presence of reflection features in the X-ray spectrum, notably a broad iron line. Fitting the data with a relativistic reflection model, we derive a disk inclination of 25 degrees. The spectral and polarization properties are comparable with other atolls observed by IXPE, suggesting a similar accretion geometry, and the relatively low polarization is consistent with the low inclination.
引用
收藏
页数:7
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