The Astrophysical Journal, 761:173 (19pp), 2012 December 20 doi:10.1088/0004-637X/761/2/173 C 2012. The American Astronomical Society. All rights reserved. Printed in the U.S.A. THE RADIO LIGHT CURVE OF THE GAMMA-RAY NOVA IN V407 CYG: THERMAL EMISSION FROM THE IONIZED SYMBIOTIC ENVELOPE, DEVOURED FROM WITHIN BY THE NOVA BLAST Laura Chomiuk1,2,3, Miriam I. Krauss1, Michael P. Rupen1, Thomas Nelson4, Nirupam Roy1, Jennifer L. Sokoloski5, Koji Mukai6,7, Ulisse Munari8, Amy Mioduszewski1, Jennifer Weston5, Tim J. O’Brien9, Stewart P. S. Eyres10, and Michael F. Bode11 1 National Radio Astronomy Observatory, P.O. Box O, Socorro, NM 87801, USA;
[email protected] 2 Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA 3 Department of Physics and Astronomy, Michigan State University, East Lansing, MI 48824, USA 4 School of Physics and Astronomy, University of Minnesota, 116 Church Street SE, Minneapolis, MN 55455, USA 5 Columbia Astrophysics Laboratory, Columbia University, New York, NY 10027, USA 6 CRESST and X-ray Astrophysics Laboratory, NASA/GSFC, Greenbelt, MD 20771, USA 7 Center for Space Science and Technology, University of Maryland Baltimore County, Baltimore, MD 21250, USA 8 INAF Astronomical Observatory of Padova, I-36012 Asiago (VI), Italy 9 Jodrell Bank Centre for Astrophysics, University of Manchester, Manchester M13 9PL, UK 10 Jeremiah Horrocks Institute, University of Central Lancashire, Preston PR1 2HE, UK 11 Astrophysics Research Institute, Liverpool John Moores University, Twelve Quays House, Egerton Wharf, Birkenhead CH41 1LD, UK Received 2012 June 23; accepted 2012 October 26; published 2012 December 5 ABSTRACT We present multi-frequency radio observations of the 2010 nova event in the symbiotic binary V407 Cygni, obtained with the Karl G.