The recent evolution of radio emission from GX 339-4

Details The recent evolution of radio emission from GX 339-4 The recent evolution of radio emission from GX 339-4

Sep 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002atel..107....1f&link_type=abstract

The Astronomer's Telegram, #107

Astronomy and Astrophysics

Astronomy

12

Radio, X-Ray, Black Holes, Transients

Scientific paper

We report on the evolution of the radio emission from the black hole candidate GX 339-4, as observed with the Australia Telescope Compact Array (ATCA). These observations are associated with the re-appearance of GX 339-4 as a bright X-ray source following approximately three years in an "Off" state, and subsequent transition to the current extremely bright X-ray state. Three sets of observations between MJD 52368-52382 revealed a radio source with an approximately flat spectrum between 1 - 9 GHz, at a level between 5 - 14 mJy, characteristic of the low/hard X-ray state.

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