An X-ray detection possibility of star-formation-bursting proto-elliptical galaxies

被引：0
|
作者：
Inoue, H [1 ]
Yamasaki, NY [1 ]
机构：
[1] Inst Space & Astronaut Sci, Sagamihara, Kanagawa 2298510, Japan
来源：
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN | 2003年 / 55卷 / 03期
关键词：
galaxies : high-redshift; galaxies : starburst; X-rays : galaxies;
D O I：
10.1093/pasj/55.3.631
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
A possibility to detect X-rays from star-formation burst activities in proto-elliptical galaxies is considered. The X-ray flux of an emission due to inverse-Compton scattering of the cosmic microwave background (CMB) by high energy electrons accelerated in SNRs is shown to increase as z increases far beyond unity, since the local CMB flux largely increases in association with a z-increase. The flux is estimated for the case of a very high rate of type 11 supernovae at an initial star formation burst of a proto-elliptical galaxy and is found to be detectable with a future large X-ray telescope such as intended in the XEUS mission.
引用
收藏
页码：631 / 634
页数：4
相关论文
共 50 条
  • [31] X-ray number counts of star forming galaxies
    Ranalli, P
    Comastri, A
    Setti, G
    MULTIWAVELENGTH AGN SURVEYS, 2004, : 43 - 44
  • [32] An X-ray detection of star formation in a highly magnified giant arc
    Bayliss, M. B.
    McDonald, M.
    Sharon, K.
    Gladders, M. D.
    Florian, M.
    Chisholm, J.
    Dahle, H.
    Mahler, G.
    Paterno-Mahler, R.
    Rigby, J. R.
    Rivera-Thorsen, E.
    Whitaker, K. E.
    Allen, S.
    Benson, B. A.
    Bleem, L. E.
    Brodwin, M.
    Canning, R. E. A.
    Chiu, I.
    Hlavacek-Larrondo, J.
    Khullar, G.
    Reichardt, C.
    Vieira, J. D.
    NATURE ASTRONOMY, 2020, 4 (02) : 159 - 166
  • [33] An X-ray detection of star formation in a highly magnified giant arc
    M. B. Bayliss
    M. McDonald
    K. Sharon
    M. D. Gladders
    M. Florian
    J. Chisholm
    H. Dahle
    G. Mahler
    R. Paterno-Mahler
    J. R. Rigby
    E. Rivera-Thorsen
    K. E. Whitaker
    S. Allen
    B. A. Benson
    L. E. Bleem
    M. Brodwin
    R. E. A. Canning
    I. Chiu
    J. Hlavacek-Larrondo
    G. Khullar
    C. Reichardt
    J. D. Vieira
    Nature Astronomy, 2020, 4 : 159 - 166
  • [34] High resolution X-ray spectroscopy and chemical evolution in elliptical galaxies
    Loewenstein, Michael
    Davis, David S.
    ADVANCES IN SPACE RESEARCH, 2008, 41 (12) : 1972 - 1974
  • [35] A fundamental plane relation for the X-ray gas in normal elliptical galaxies
    Diehl, S
    Statler, TS
    ASTROPHYSICAL JOURNAL, 2005, 633 (01): : L21 - L24
  • [36] X-Ray Measurements of the Mass Profiles in Massive Isolated Elliptical Galaxies
    Buote, David A.
    O'Sullivan, Ewan
    Ponman, Trevor J.
    GALAXY MASSES AS CONSTRAINTS OF FORMATION MODELS, 2015, 10 (311): : 40 - 44
  • [37] Gas dynamic stripping and X-ray emission of cluster elliptical galaxies
    Toniazzo, T
    Schindler, S
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2001, 325 (02) : 509 - 530
  • [38] Hydrodynamical model of X-ray emitting gas around elliptical galaxies
    Saito, R
    Shigeyama, T
    HOT UNIVERSE, 1998, (188): : 286 - 286
  • [39] High-mass X-ray binaries as a star formation rate indicator in distant galaxies
    Grimm, HJ
    Gilfanov, M
    Sunyaev, R
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2003, 339 (03) : 793 - 809
  • [40] THE HOST GALAXIES OF X-RAY QUASARS ARE NOT STRONG STAR FORMERS
    Barger, A. J.
    Cowie, L. L.
    Owen, F. N.
    Chen, C. -C.
    Hasinger, G.
    Hsu, L. -Y.
    Li, Y.
    ASTROPHYSICAL JOURNAL, 2015, 801 (02):
12345