The EVLA Nova Project: A New Window on Radio Emission from Galactic Novae

Details The EVLA Nova Project: A New Window on Radio Emission from Galactic Novae The EVLA Nova Project: A New Window on Radio Emission from Galactic Novae

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011head...12.1101k&link_type=abstract

American Astronomical Society, HEAD meeting #12, #11.01

Astronomy and Astrophysics

Astronomy

Scientific paper

The EVLA Nova Team is embarking on a new era of radio observations of novae, inspired by the more than order-of-magnitude improvement in sensitivity and enhanced frequency coverage of the EVLA. We present results from our first 1.5 years of observations, which includes wide-band (1--50 GHz) monitoring of three sources: V407 Cyg, V1723 Aql, and T Pyx. None of these objects have radio characteristics conforming to the simple canonical model of expanding, spherical, thermally-emitting ejecta. In addition to our radio observations, we consider contemporaneous high-energy observations of these novae, and discuss possible physical mechanisms for the production of the observed radio emission.

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