GINGA OBSERVATIONS OF SEYFERT-GALAXIES

被引:35
作者
AWAKI, H [1 ]
KOYAMA, K [1 ]
机构
[1] KYOTO UNIV,DEPT PHYS,SAKYO KU,KYOTO 606,JAPAN
来源
SPACE ASTRONOMY | 1993年 / 13卷 / 12期
关键词
D O I
10.1016/0273-1177(93)90114-Q
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
We observed twenty-eight Seyfert 2 galaxies with the Japanese X-ray satellite, Ginga, and found Seyfert 2 galaxies, in general, have the X-ray spectral characteristics of obscured Seyfert 1 nuclei. This result agrees with the predictions from Unified Seyfert model proposed by Antonucci and Miller/1/. However, among the observed Seyfert 2 galaxies, there are a few galaxies with no evidence of an obscuration, contrary to the general predictions of the unified model. We note that type 2 AGN will contribute to the Cosmic Diffuse X-ray Background, if the unified Seyfert model can be extended to the far distant AGN such as quasars.
引用
收藏
页码:221 / 230
页数:10
相关论文
共 31 条
  • [1] SPECTROPOLARIMETRY AND THE NATURE OF NGC-1068
    ANTONUCCI, RRJ
    MILLER, JS
    [J]. ASTROPHYSICAL JOURNAL, 1985, 297 (02) : 621 - 632
  • [2] AWAKI H, 1991, PUBL ASTRON SOC JPN, V43, P195
  • [3] AWAKI H, 1991, PUBL ASTRON SOC JPN, V43, pL37
  • [4] X-RAY EVIDENCE OF AN OBSCURED NUCLEUS IN THE TYPE-2 SEYFERT-GALAXY MKN3
    AWAKI, H
    KOYAMA, K
    KUNIEDA, H
    TAWARA, Y
    [J]. NATURE, 1990, 346 (6284) : 544 - 545
  • [5] AWAKI H, 1992, NATURE
  • [6] AWAKI H, 1991, THESIS NAGOYA U
  • [7] AWAKI H, 1992, COMMUNICATION
  • [8] IRON K-SHELL EMISSION FROM NGC-1068
    BAND, DL
    KLEIN, RI
    CASTOR, JI
    NASH, JK
    [J]. ASTROPHYSICAL JOURNAL, 1990, 362 (01) : 90 - 99
  • [9] BRINDLE C, 1990, MON NOT R ASTRON SOC, V244, P577
  • [10] X-RAY-BACKGROUND, DISCRETE SOURCES, AND DIFFUSE PROCESSES
    GIACCONI, R
    ZAMORANI, G
    [J]. ASTROPHYSICAL JOURNAL, 1987, 313 (01) : 20 - 27