Radio synchrotron emission from V2672 Oph

Details Radio synchrotron emission from V2672 Oph Radio synchrotron emission from V2672 Oph

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009atel.2195....1k&link_type=abstract

The Astronomer's Telegram, #2195

Astronomy and Astrophysics

Astronomy

3

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

Scientific paper

Very Large Array (VLA) C configuration observations of the fast nova V2672 Oph (IAUC 9064; ATel #2173) at 8.46 GHz on 1 September 2009 (MJD 55075.13; 15.61 days after the optical discovery [IAUC
9064]) detect an unresolved source 0.65 arcsec from the reported optical position, with a flux density of 0.526 +/- 0.033 mJy.

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