EVLA Radio Upper Limits on Nova V5587 Sgr

Details EVLA Radio Upper Limits on Nova V5587 Sgr EVLA Radio Upper Limits on Nova V5587 Sgr

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3227....1c&link_type=abstract

The Astronomer's Telegram, #3227

Astronomy and Astrophysics

Astronomy

Radio, Nova

Scientific paper

We observed the nova V5587 Sgr (CBET 2644, IAUC 9196) with the EVLA on three dates ranging from 8 to 40 days after discovery (2011 Jan 25.9); all observations yielded non-detections. Below are the UT dates, flux density measurements with 1-sigma uncertainties, and lower limits on the distance. The distance limits derive from the assumption that the radio emission is thermal free-free emission from an optically thick expanding sphere with a temperature of 104 K and a radius that increases at a rate of 1650 km/s.

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