Observations with the ATCA of the brightest known radio hard state in GX 339-4

Details Observations with the ATCA of the brightest known radio hard state in GX 339-4 Observations with the ATCA of the brightest known radio hard state in GX 339-4

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2525....1c&link_type=abstract

The Astronomer's Telegram, #2525

Astronomy and Astrophysics

Astronomy

2

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

Scientific paper

The recurrent black hole candidate GX 339-4 has entered a new outburst early this year (ATel #2380). It has continuously been observed in the hard state (ATel #2384, #2455, #2459), that is typically observed in the rising part of the outburst. Since its reactivation, we have been monitoring GX 339-4 very frequently in radio with the Australia Telescope Compact Array and the new CABB back-end (mostly at 5.5 GHz and 9 GHz).

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