Radio and X-ray observations of GX 339-4Observations of the Galactic black hole candidate binary system GX 339-4 at radio, optical and X-ray wavelengths are reviewed. The radio observations reveal a compact, persistent and variable source. On the average, the radio intensity is less than 10 mJy. These data, when compared with previous data, indicate no set correlation between the radio and X-ray emission. The X-ray intensity suggests a 14.5 month cycle. The latest radio observational data are presented together with X-ray data and are discussed in the context of similar correlated observations from other X-ray binaries.
Document ID
19970025762
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Sood, R. (Australian Defence Force Academy Canberra Australia)
Durouchoux, P. (Commissariat a l'Energie Atomique Saclay France)
Campbell-Wilson, D. (Sydney Univ. Australia)
Vilhu, O. (Helsinki Univ. Helsinki Finland)
Wallyn, P. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Date Acquired
August 17, 2013
Publication Date
March 1, 1997
Publication Information
Publication: Proceedings of 2nd INTEGRAL Workshop 'The Transparent Universe'