共 50 条
Suzaku observation of the anomalous X-ray pulsar CXOU J164710.2-455216
被引:8
|作者:
Naik, Sachindra
[1
]
Dotani, Tadayasu
[1
,2
,3
]
Kawai, Nobuyuki
[3
]
Kokubun, Motohide
[1
]
Anada, Takayasu
[1
]
Morii, Mikio
[4
]
Mihara, Tatehiro
[5
]
Enoto, Teruaki
[6
]
Kawaharada, Madoka
[6
]
Murakami, Toshio
[7
]
Nakagawa, Yujin E.
[8
]
Takahashi, Hiromitsu
[9
]
Terada, Yukikatsu
[5
]
Yoshida, Atsumasa
[8
]
机构:
[1] Japan Aerosp Explorat Agcy, Inst Space & Astronaut Sci, Sagamihara, Kanagawa 2298510, Japan
[2] Grad Univ Adv Studies, Sch Phys Sci, Sagamihara, Kanagawa 2298510, Japan
[3] Tokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo 1528551, Japan
[4] Rikkyo Univ, Dept Phys, Toshima Ku, Tokyo 1718501, Japan
[5] Inst Phys & Chem Res, Cosm Radiat Lab, Wako, Saitama 3510198, Japan
[6] Univ Tokyo, Dept Phys, Bunkyo Ku, Tokyo 1130033, Japan
[7] Kanazawa Univ, Dept Phys, Kanazawa, Ishikawa 9201192, Japan
[8] Aoyama Gakuin Univ, Grad Sch Sci & Engn, Kanagawa 2298558, Japan
[9] Hiroshima Univ, Dept Phys Sci, Hiroshima 7398526, Japan
关键词:
stars : neutron;
stars : pulsars : individual (CXOU J164710.2-455216);
X-rays : general;
X-rays : individual (CXOU J164710.2-455216);
D O I:
10.1093/pasj/60.2.237
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
A Suzaku TOO observation of CXOU J164710.2-455216 was performed on 2006 September 23-24 for a net exposure of 38.8 ks. Pulsations were clearly detected in the XIS light curves with a pulse period of 10.61063(2) s. The XIS pulse profile is found to be highly non-sinusoidal. It shows 3 peaks of different amplitudes with an RMS fractional amplitude of similar to 11% in the 0.2-6.0 keV energy band. The 1 -10 keV XIS spectra were well fitted by two different models consisting of a power-law and a blackbody component and two blackbody components, respectively. Although both the models are statistically acceptable, a difference in the pulse profiles at soft (0.2-6.0 keV) and hard (6-12keV) X-rays favors the model consisting of two blackbody components. The temperatures of two blackbody components are found to be 0.61 +/- 0.01 keV and 1.22 +/- 0.06 keV, and the value of the absorption column density is 1.73 +/- 0.03 x 10(22) atoms cm(-2). Pulse phase resolved spectroscopy shows that the flux of the soft blackbody component consists of three narrow peaks, whereas the flux of the other component shows a single peak over the pulse period of the AXP. The blackbody radii change between 2.2-2.7 km and 0.28-0.38 km (assuming the source distance to be 5 kpc) over the pulse phases for the soft and hard components, respectively. The details of the results obtained from the timing and spectral analyses are presented.
引用
收藏
页码:237 / 244
页数:8
相关论文