The radio counterpart of the X-ray pulsar wind nebula in the SNR G0.9+0.1

被引：0
|
作者：
Dubner, G [1 ]
Giacani, E
Decourchelle, A
机构：
[1] Inst Astron & Space Phys, Buenos Aires, DF, Argentina
[2] CEA Saclay, Serv Astrophys, Saclay, France
来源：
PROCEEDINGS OF THE X-RAY UNIVERSE 2005, VOLS 1 AND 2 | 2006年 / 604卷
关键词：
X-rays; radio continuum; supernova remnants; G0.9+0.1;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We report on new radio observations of the central nebula in the SNR G0.9+0.1 at 4.8 GHz and 8.6 GHz. These data unveil a highly clumpy structure of the radio nebula. Most of the radio features are uncorrelated with the X-ray emission. Not any point-like radio source is detected at the position of CXOU J174722.8-280915, the proposed neutron star. On the contrary, the X-ray source seems to lie within a small minimum in the radio emission.
引用
收藏
页码：365 / +
页数：2
相关论文
共 50 条
  • [21] Discovery of X-ray emission from a radio supernova remnant G352.7-0.1
    Kinugasa, K
    Torii, K
    Tsunemi, H
    Yamauchi, S
    Koyama, K
    Dotani, T
    PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 1998, 50 (02) : 249 - 255
  • [22] The radio emission, X-ray emission, and hydrodynamics of G328.4+0.2: A comprehensive analysis of a luminous pulsar wind nebula, its neutron star, and the progenitor supernova explosion
    Gelfand, Joseph D.
    Gaensler, B. M.
    Slane, Patrick O.
    Patnaude, Daniel J.
    Hughes, John P.
    Camilo, Fernando
    ASTROPHYSICAL JOURNAL, 2007, 663 (01) : 468 - 486
  • [23] HIGH-RESOLUTION X-RAY OBSERVATIONS OF THE PULSAR WIND NEBULA ASSOCIATED WITH THE GAMMA-RAY SOURCE HESSJ 1640-465
    Lemiere, A.
    Slane, P.
    Gaensler, B. M.
    Murray, S.
    ASTROPHYSICAL JOURNAL, 2009, 706 (02) : 1269 - 1276
  • [24] The X-ray jet in the Crab nebula: Radical implications for pulsar theory?
    Lyubarsky, Y
    Eichler, D
    ASTROPHYSICAL JOURNAL, 2001, 562 (01) : 494 - 498
  • [25] THE RADIO COUNTERPART TO THE LUMINOUS X-RAY SUPERNOVA REMNANT IN NGC-6946
    VANDYK, SD
    SRAMEK, RA
    WEILER, KW
    HYMAN, SD
    VIRDEN, RE
    ASTROPHYSICAL JOURNAL, 1994, 425 (02) : L77 - L79
  • [26] THE EVOLUTION OF THE γ- AND X-RAY LUMINOSITIES OF PULSAR WIND NEBULAE
    Mattana, F.
    Falanga, M.
    Goetz, D.
    Terrier, R.
    Esposito, P.
    Pellizzoni, A.
    De Luca, A.
    Marandon, V.
    Goldwurm, A.
    Caraveo, P. A.
    ASTROPHYSICAL JOURNAL, 2009, 694 (01) : 12 - 17
  • [27] RETRACTED ARTICLE: X-ray observations of PSR B0355+54 and its pulsar wind nebula
    Katherine E. McGowan
    W. Thomas Vestrand
    Jamie A. Kennea
    Silvia Zane
    Mark Cropper
    France A. Córdova
    Astrophysics and Space Science, 2007, 308 : 309 - 316
  • [28] THE RADIO COUNTERPART OF THE HARD X-RAY SOURCE GRS-1758-258
    RODRIGUEZ, LF
    MIRABEL, IF
    MARTI, J
    ASTROPHYSICAL JOURNAL, 1992, 401 (01) : L15 - L18
  • [29] Discovery of a new X-ray filled radio supernova remnant around the pulsar wind nebula in 3EG J1809-2328
    Roberts, Mallory S. E.
    Brogan, Crystal L.
    ASTROPHYSICAL JOURNAL, 2008, 681 (01) : 320 - 324
  • [30] Discovery of an X-ray synchrotron nebula associated with the radio pulsar PSR B1853+01 in the supernova remnant W44
    Harrus, IM
    Hughes, JP
    Helfand, DJ
    ASTROPHYSICAL JOURNAL, 1996, 464 (02) : L161 - &
12345