Kepler's supernova remnant: The view at 400 years

被引:0
|
作者
Blair, WP [1 ]
机构
[1] Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA
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
October 2004 marks the 400th anniversary of the sighting of SN 1604, now marked by the presence of an expanding nebulosity known as Kepler's supernova remnant. Of the small number of remnants of historical supernovae, Kepler's remnant remains the most enigmatic. The supernova type, and hence the type of star that exploded, is still a matter of debate, and even the distance to the remnant is uncertain by more than a factor of two. As new and improved multiwavength observations become available, and as the time baseline of observations gets longer, Kepler's supernova remnant is slowly revealing its secrets. I review recent and current observations of Kepler's supernova, remnant,and what they indicate about this intriguing object.
引用
收藏
页码:416 / 421
页数:6
相关论文
共 50 条
  • [21] A 3D numerical model for Kepler's supernova remnant
    Toledo-Roy, J. C.
    Esquivel, A.
    Velazquez, P. F.
    Reynoso, E. M.
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2014, 442 (01) : 229 - 238
  • [22] Emission of Kepler's supernova remnant produced by accelerated cosmic rays
    Berezhko, E. G.
    Ksenofontov, L. T.
    Voelk, H. J.
    Yelshin, V. K.
    Proceedings of the 29th International Cosmic Ray Conference, Vol 4: OG 2.1, 2.2 & 2.3, 2005, : 227 - 230
  • [23] The imprint of a symbiotic binary progenitor on the properties of Kepler's supernova remnant
    Chiotellis, A.
    Schure, K. M.
    Vink, J.
    ASTRONOMY & ASTROPHYSICS, 2012, 537
  • [24] HSTACS imaging of a Balmer-dominated shock in Kepler's supernova remnant
    Sankrit, R
    Blair, WP
    DeLaney, T
    Rudnick, L
    Harrus, IM
    Ennis, JA
    YOUNG NEUTRON STARS AND SUPERNOVA REMNANTS, 2005, 35 (06): : 1027 - 1030
  • [25] Accounting for the foreground contribution to the dust emission towards Kepler's supernova remnant
    Gomez, H. L.
    Dunne, L.
    Ivison, R. J.
    Reynoso, E. M.
    Thompson, M. A.
    Sibthorpe, B.
    Eales, S. A.
    DeLaney, T. M.
    Maddox, S.
    Isaak, K.
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2009, 397 (03) : 1621 - 1632
  • [26] Gamma-ray emission expected from Kepler's supernova remnant
    Berezhko, E. G.
    Ksenofontov, L. T.
    Voelk, H. J.
    ASTRONOMY & ASTROPHYSICS, 2006, 452 (01): : 217 - 221
  • [27] Gamma-ray emission expected from Kepler's supernova remnant
    Berezhko, E.G.
    Ksenofontov, L.T.
    Völk, H.J.
    Astronomy and Astrophysics, 1600, 452 (01): : 217 - 221
  • [28] Radio spectral index variations and physical conditions in Kepler's supernova remnant
    DeLaney, T
    Koralesky, B
    Rudnick, L
    Dickel, JR
    ASTROPHYSICAL JOURNAL, 2002, 580 (02): : 914 - 927
  • [29] Dust-to-gas ratios in the Kepler supernova remnant
    Contini, M
    ASTRONOMY & ASTROPHYSICS, 2004, 422 (02) : 591 - 602
  • [30] ON THE X-RAY-SPECTRUM OF KEPLER SUPERNOVA REMNANT
    BORKOWSKI, KJ
    SARAZIN, CL
    BLONDIN, JM
    ASTROPHYSICAL JOURNAL, 1994, 429 (02): : 710 - 725