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-Reference-Cited by-同舟云学术

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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

Published:2012-12-05 Issue:2 Volume:761 Page:173
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Chomiuk Laura,Krauss Miriam I.,Rupen Michael P.,Nelson Thomas,Roy Nirupam,Sokoloski Jennifer L.,Mukai Koji,Munari Ulisse,Mioduszewski Amy,Weston Jennifer,O'Brien Tim J.,Eyres Stewart P. S.,Bode Michael F.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/761/i=2/a=173/pdf

Reference118 articles.

1. Mass loss from very luminous OB stars and the Cygnus superbubble

2. Gamma-Ray Emission Concurrent with the Nova in the Symbiotic Binary V407 Cygni

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