MITSuME observation of V404 Cygni in the 2015 outburst: Two optical variable components with different variability
Author:
Affiliation:
1. Department of Physics, Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro-ku, Tokyo 152-8551, Japan
2. Ishigakijima Astronomical Observatory, National Astronomical Observatory of Japan, 1024-1 Arakawa, Ishigaki, Okinawa 907-0024, Japan
Funder
MEXT
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/pasj/article-pdf/69/4/63/19489172/psx040.pdf
Reference57 articles.
1. A 6.5-day periodicity in the recurrent nova V404 Cygni implying the presence of a black hole
2. Revisiting a fundamental test of the disc instability model for X-ray binaries
3. Evidence for a Disk-Jet Interaction in the Microquasar GRS 1915+105
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