A New X-Ray Spectro-Temporal Analysis Method and Its Application to the Suzaku MCG-6-30-15 Data

被引:3
作者
Inoue, Hajime [1 ]
Miyakawa, Takehiro [1 ,2 ]
Ebisawa, Ken [1 ,2 ]
机构
[1] Japan Aerosp Exporlat Agcy JAXA, ISAS, Chuo Ku, Sagamihara, Kanagawa 2525210, Japan
[2] Univ Tokyo, Grad Sch Sci, Dept Astron, Bunkyo Ku, Tokyo 1130033, Japan
关键词
galaxies: active; galaxies: individual (MCG-6-30-15); galaxies: Seyfert; X-rays: galaxies; SEYFERT-1 GALAXY MCG-6-30-15; IRON LINE; VARIABILITY; MODEL; EMISSION; DISK;
D O I
10.1093/pasj/63.sp3.S669
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A new X-ray spectro-temporal data-analysis method, which we call "the difference variation function method", is introduced. It can analyze spectral and temporal variations of X-ray sources, and its merits are discussed in comparison with conventional data-analysis methods. The new method is being applied to Suzaku observation data of the Seyfert 1 galaxy MCG -6-30-15. Consequently, it has been found that the observed spectral and temporal variations on a time scale of approximate to 10-100 ks are mostly ascribed to variable partially absorbers in front of the central X-ray source, whereas the X-ray source is intrinsically variable mainly on time scales shorter than approximate to 10 ks.
引用
收藏
页码:S669 / S675
页数:7
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