The hardest X-ray source in the ASCA large sky survey:: Discovery of a new type 2 Seyfert

被引:10
作者
Sakano, M [1 ]
Koyama, K
Tsuru, T
Awaki, H
Ueda, Y
Takahashi, T
Akiyama, M
Ohta, K
Yamada, T
机构
[1] Kyoto Univ, Dept Phys, Kyoto 6068502, Japan
[2] Inst Space & Astronaut Sci, Kanagawa 2298510, Japan
[3] Kyoto Univ, Dept Astron, Kyoto 6068502, Japan
[4] Tohoku Univ, Inst Astron, Sendai, Miyagi 9808578, Japan
关键词
diffuse radiation; galaxies : active; galaxies : individual (AX J131501+3141) galaxies : Seyfert; X-rays : galaxies;
D O I
10.1086/306158
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present results of the ASCA deep-exposure observations of the hardest X-ray source discovered in the ASCA Large Sky Survey (LSS) project, designated as AX J131501 + 3141. We extract its accurate X-ray spectrum, taking into account the contamination from a nearby soft source (AX J131502 + 3142) separated from it by only 1'. AX J131501 + 3141 exhibits a large absorption of N-H = 6(-2)(+4) x 10(22) H cm(-2), with a photon index Gamma = 1.5(-0.6)(+0.7). The 2-10 keV flux was about 5 x 10(-13) ergs cm(-2) s(-1), and was time variable by a factor of 30% in 0.5 yr. From the highly absorbed X-ray spectrum and the time variability, as well as the results of the optical follow-up observations, we conclude that AX J131501 + 3141 is a type 2 Seyfert galaxy. Discovery of such a low-flux and highly absorbed X-ray source could have a significant impact on our understanding of the origin of the cosmic X-ray background.
引用
收藏
页码:129 / 133
页数:5
相关论文
共 31 条
[1]   Optical identification of the hardest X-ray source in the ASCA large sky survey [J].
Akiyama, M ;
Ohta, K ;
Yamada, T ;
Eracleous, M ;
Halpern, JP ;
Kashikawa, N ;
Yagi, M ;
Kawasaki, W ;
Sakano, M ;
Tsuru, T ;
Ueda, Y ;
Takahashi, T .
ASTROPHYSICAL JOURNAL, 1998, 500 (01) :173-180
[2]   UNIFIED MODELS FOR ACTIVE GALACTIC NUCLEI AND QUASARS [J].
ANTONUCCI, R .
ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, 1993, 31 :473-521
[3]  
AWAKI H, 1991, PUBL ASTRON SOC JPN, V43, P195
[4]  
AWAKI H, 1991, THESIS NAGOYA U
[5]   CCD SOFT-X-RAY IMAGING SPECTROMETER FOR THE ASCA SATELLITE [J].
BURKE, BE ;
MOUNTAIN, RW ;
DANIELS, PJ ;
COOPER, MJ ;
DOLAT, VS .
IEEE TRANSACTIONS ON NUCLEAR SCIENCE, 1994, 41 (01) :375-385
[6]   AN ABUTTABLE CCD IMAGER FOR VISIBLE AND X-RAY FOCAL PLANE ARRAYS [J].
BURKE, BE ;
MOUNTAIN, RW ;
HARRISON, DC ;
BAUTZ, MW ;
DOTY, JP ;
RICKER, GR ;
DANIELS, PJ .
IEEE TRANSACTIONS ON ELECTRON DEVICES, 1991, 38 (05) :1069-1076
[7]  
COMASTRI A, 1995, ASTRON ASTROPHYS, V296, P1
[8]  
DAY C, 1995, ABC GUIDE ASCA DATA
[9]   Ion-supported tori: A thermal bremsstrahlung model for the X-ray background [J].
DiMatteo, T ;
Fabian, AC .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1997, 286 (02) :393-402
[10]  
FABIAN AC, 1992, ANNU REV ASTRON ASTR, V30, P429