On the nature of V630 Cassiopeiae

Details On the nature of V630 Cassiopeiae On the nature of V630 Cassiopeiae

Dec 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.222..225w&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 222, no. 1-2, p. 225-226

Astronomy and Astrophysics

Astrophysics

4

Cassiopeia Constellation, Cataclysmic Variables, Dwarf Novae, Orbital Mechanics, Accretion Disks, Flux Density, Light Curve, Periodic Functions, Stellar Magnitude

Scientific paper

From its similarity to BV Cen, GK Per and V1017 Sgr it is suggested that
V630 Cas may be a rare example of a dwarf nova with a long orbital
period.

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