X-ray emission from the Galactic ridge

被引：0
作者：
Tanaka, Y [1 ]
机构：
[1] Inst Space & Astronaut Sci, Sagamihara, Kanagawa 229, Japan
来源：
NEW CENTURY OF X-RAY ASTRONOMY | 2001年 / 251卷
关键词：
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The recent Chandra result confirmed that most of the Galactic ridge X-ray emission is diffuse emission. Thermal plasma interpretations of the emission seem to contain fundamental problems. These are discussed together with the reanalysis results of the ASCA data.
引用
收藏
页码：40 / 44
页数：5
相关论文
共 12 条
  • [1] Complex spectra of the galactic ridge X-rays observed with ASCA
    Kaneda, H
    Makishima, K
    Yamauchi, S
    Koyama, K
    Matsuzaki, K
    Yamasaki, NY
    [J]. ASTROPHYSICAL JOURNAL, 1997, 491 (02) : 638 - 652
  • [2] KANEDA H, 1997, 642 ISAS RN
  • [3] ASCA view of our galactic center: Remains of past activities in X-rays?
    Koyama, K
    Maeda, Y
    Sonobe, T
    Takeshima, T
    Tanaka, Y
    Yamauchi, S
    [J]. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 1996, 48 (02) : 249 - 255
  • [4] MAKISHIMA K, 1997, XRAY IMAGING SPECTRO, P137
  • [5] Interstellar abundances from absorption-line observations with the Hubble Space Telescope
    Savage, BD
    Sembach, KR
    [J]. ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, 1996, 34 : 279 - 329
  • [6] Unusual properties of X-ray emission near the Galactic center
    Tanaka, Y
    Koyama, K
    Maeda, Y
    Sonobe, T
    [J]. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 2000, 52 (04) : L25 - L30
  • [7] Tanaka Y, 1999, ASTRON NACHR, V320, P181, DOI 10.1002/1521-3994(199908)320:4/5<181::AID-ASNA181>3.0.CO
  • [8] 2-#
  • [9] Magnetic reconnection as the origin of galactic-ridge x-ray emission
    Tanuma, S
    Yokoyama, T
    Kudoh, T
    Matsumoto, R
    Shibata, K
    Makishima, K
    [J]. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 1999, 51 (01) : 161 - 171
  • [10] Measurement of the galactic X-ray/gamma-ray background radiation: Contribution of discrete sources
    Valinia, A
    Kinzer, RL
    Marshall, FE
    [J]. ASTROPHYSICAL JOURNAL, 2000, 534 (01) : 277 - 282
12