The optical observations of X ray Nova GS2023+33 = V404 CYG

Details The optical observations of X ray Nova GS2023+33 = V404 CYG The optical observations of X ray Nova GS2023+33 = V404 CYG

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990esasp.311..301o&link_type=abstract

In ESA, Plasma Astrophysics p 301-302 (SEE N91-15046 06-90)

Astronomy and Astrophysics

Astrophysics

1

Accretion Disks, Novae, Photometry, Stellar Mass Accretion, X Ray Binaries, Bursts, Comparison

Scientific paper

The results of optical observations of Nova V404 Cyg 1989 are presented in comparison with the outburst in 1938. A possible model in the framework of nonstationary disk accretion is compared with that for Nova Vul 1988. Conclusions include that the outer disk radius in V404 is larger. The system V404 seems to be wider in comparison with Nova Vul 1988.

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