EVLA monitoring of V407 Cyg

Details EVLA monitoring of V407 Cyg EVLA monitoring of V407 Cyg

Jul 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2741....1k&link_type=abstract

The Astronomer's Telegram, #2741

Astronomy and Astrophysics

Astronomy

1

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.

Affiliated with

Also associated with

No associations

Rating

EVLA monitoring of V407 Cyg does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with EVLA monitoring of V407 Cyg, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and EVLA monitoring of V407 Cyg will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-954647