e-VLBI detection of Circinus X-1 at 1.6 and 8.4 GHz

Details e-VLBI detection of Circinus X-1 at 1.6 and 8.4 GHz e-VLBI detection of Circinus X-1 at 1.6 and 8.4 GHz

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007atel.1037....1d&link_type=abstract

The Astronomer's Telegram, #1037

Astronomy and Astrophysics

Astronomy

2

Radio, Binaries, Neutron Stars, Transients

Scientific paper

Following the return of Circinus X-1 to a recurrent radio flaring state (last seen in 1975 - 1985: ATel #563, #985) we have performed e-VLBI observations on the source at 1.6 and 8.4 GHz using an Australian array of radio telescopes (Parkes, ATCA, Mopra, and Hobart). e-VLBI allows rapid response to transient events and real-time analysis of VLBI data, in this case implemented by transfer of data between telescopes via optical fibres and software correlation on a PC cluster.

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