Witnessing with the ATCA the interaction of a relativistic jet from GX 339-4 with the interstellar medium

Details Witnessing with the ATCA the interaction of a relativistic jet from GX 339-4 with the interstellar medium Witnessing with the ATCA the interaction of a relativistic jet from GX 339-4 with the interstellar medium

Jul 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2745....1c&link_type=abstract

The Astronomer's Telegram, #2745

Astronomy and Astrophysics

Astronomy

2

Radio, Infra-Red, Optical, X-Ray, Request For Observations, Black Holes, Transients

Scientific paper

We conducted radio observations (at 5.5 GHz and 9 GHz) of GX 339-4 on 2010 June 25 with the ATCA (Australia Telescope Compact Array) and the new CABB back-end. No radio emission is detected at the location of GX 339-4, which is consistent with the source being in the soft state. However, we notice a new radio source located very close to the core of the system, with radio flux density of 2.39 ± 0.06 mJy at 5.5 GHz and 2.02 ± 0.06 mJy at 9 GHz.

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