A Light Curve Analysis of Recurrent and Very Fast Novae in Our Galaxy, Magellanic Clouds, and M31
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4365/aac833/pdf
Reference173 articles.
1. Gamma-Ray Emission Concurrent with the Nova in the Symbiotic Binary V407 Cygni
2. Fermi establishes classical novae as a distinct class of gamma-ray sources
3. The 1999 Outburst of the Recurrent Nova U Scorpii
4. The 2010 outburst and pre-outburst optical spectrum of the recurrent nova U Scorpii
5. Multiwavelength observations of nova SMCN 2016-10a – one of the brightest novae ever observed
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