High-resolution radio observations of the black hole candidate GX 339-4

被引:32
|
作者
Fender, RP
Spencer, RE
Newell, SJ
Tzioumis, AK
机构
[1] UNIV MANCHESTER,NUFFIELD RADIO ASTRON LABS,JODRELL BANK,MACCLESFIELD SK11 9DL,CHESHIRE,ENGLAND
[2] CSIRO,AUSTRALIA TELESCOPE NATL FACIL,EPPING,NSW 2121,AUSTRALIA
关键词
binaries; close; stars; individual; GX; 339-4; radio continuum;
D O I
10.1093/mnras/286.2.L29
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present radio observations of the black hole candidate X-ray binary GX 339-4 with the Australia Telescope Compact Array. Mapping of the highest resolution 3.5-cm data reveals a jet-like extension, which if confirmed would be the first detection of a radio jet from a persistent black hole candidate system. No evidence is found for associated structures such as bowshocks or jet lobes on larger scales. The spectral energy distribution from 22 to 3 cm is relatively flat, suggesting that emission is dominated by a compact absorbed core.
引用
收藏
页码:L29 / L32
页数:4
相关论文
共 50 条
  • [41] Constraining the mass of the black hole GX 339-4 using spectro-temporal analysis of multiple outbursts
    Sreehari, H.
    Iyer, Nirmal
    Radhika, D.
    Nandi, Anuj
    Mandal, Samir
    [J]. ADVANCES IN SPACE RESEARCH, 2019, 63 (03) : 1374 - 1386
  • [42] Internal shocks driven by accretion flow variability in the compact jet of the black hole binary GX 339-4
    Drappeau, S.
    Malzac, J.
    Belmont, R.
    Gandhi, P.
    Corbel, S.
    [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2015, 447 (04) : 3832 - 3839
  • [43] Physical Constraints from Near-infrared Fast Photometry of the Black Hole Transient GX 339-4
    Vincentelli, F. M.
    Casella, P.
    Petrucci, P.
    Maccarone, T.
    Russell, D. M.
    Uttley, P.
    De Marco, B.
    Fender, R.
    Gandhi, P.
    Malzac, J.
    O'Brien, K.
    Tomsick, J. A.
    [J]. ASTROPHYSICAL JOURNAL LETTERS, 2019, 887 (01)
  • [44] A systematic look at the very high and low/hard state of GX 339-4: constraining the black hole spin with a new reflection model
    Reis, R. C.
    Fabian, A. C.
    Ross, R. R.
    Miniutti, G.
    Miller, J. M.
    Reynolds, C.
    [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2008, 387 (04) : 1489 - 1498
  • [45] OBSERVATIONS OF HIGHLY VARIABLE X-RAY SOURCE GX 339-4
    MARKERT, TH
    CANIZARES, CR
    CLARK, GW
    LEWIN, WHG
    SCHNOPPER, HW
    SPROTT, GF
    [J]. ASTROPHYSICAL JOURNAL, 1973, 184 (02): : L67 - L70
  • [46] A jet model for the fast IR variability of the black hole X-ray binary GX 339-4
    Malzac, Julien
    Kalamkar, Maithili
    Vincentelli, Federico
    Vue, Alexis
    Drappeau, Samia
    Belmont, Renaud
    Casella, Piergiorgio
    Clavel, Maica
    Corbel, Stphane
    Coriat, Mickael
    Dornic, Damien
    Ferreira, Jonathan
    Henri, Gilles
    Maccarone, Thomas J.
    Marcowith, Alexandre
    O'Brien, Kieran
    Peault, Mathias
    Petrucci, Pierre-Olivier
    Rodriguez, Jerome
    Russell, David M.
    Uttley, Phil
    [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2018, 480 (02) : 2054 - 2071
  • [47] High-resolution X-Ray Spectroscopy of Interstellar Iron toward Cygnus X-1 and GX 339-4
    Corrales, Lia
    Gotthelf, Eric V.
    Gatuzz, Efrain
    Kallman, Timothy R.
    Lee, Julia C.
    Martins, Michael
    Paerels, Frits
    Psaradaki, Ioanna
    Schippers, Stefan
    Savin, Daniel Wolf
    [J]. ASTROPHYSICAL JOURNAL, 2024, 965 (02):
  • [48] Time evolution of the high-energy parameters of GX 339-4
    Motta, Sara
    Belloni, Tomaso M.
    [J]. X-RAY ASTRONOMY-2009: PRESENT STATUS, MULTI-WAVELENGTH APPROACH AND FUTURE PERSPECTIVES, PROCEEDINGS, 2010, 1248 : 185 - +
  • [49] Peak luminosities of the hard states of gx 339-4: Implications for the accretion geometry, disk mass, and black hole mass
    Yu, Wenfei
    Lamb, Frederick K.
    Fender, Rob
    van der Klis, Michiel
    [J]. ASTROPHYSICAL JOURNAL, 2007, 663 (02): : 1309 - 1314
  • [50] Radio/X-ray correlation in the low/hard state of GX 339-4
    Corbel, S
    Nowak, MA
    Fender, RP
    Tzioumis, AK
    Markoff, S
    [J]. ASTRONOMY & ASTROPHYSICS, 2003, 400 (03) : 1007 - 1012