EVLA monitoring of V407 Cyg

Astronomy and Astrophysics – Astronomy

Scientific paper

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Radio, Binaries, Cataclysmic Variables, Novae, Transients, Variables

Scientific paper

We report on EVLA monitoring of the symbiotic system V407 Cyg following its recent nova outburst, which has been detected from radio to gamma-ray energies (see ATels #2487, #2506, #2511, #2514, #2529, #2536, and #2546). EVLA monitoring began on 2010 April 3, approximately 3 weeks after the start of the optical outburst (CBET #2199), with observation epochs spaced by several days to ~ 2 weeks. The frequency coverage of these observations is 1.4-45 GHz, and we detect V407 Cyg at all times and all frequencies, with flux densities of 3-65 mJy.

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