A Recent Study of V783 Cygni

Details A Recent Study of V783 Cygni A Recent Study of V783 Cygni

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991javso..20..214c&link_type=abstract

The Journal of the American Association of Variable Star Observers, vol. 20, no. 2, p. 214-216

Physics

1

V783 Cygni

Scientific paper

The addition of recent observations to earlier data lead to the conclusion that a single parabolic O-C curve may explain the past behavior of the RR Lyrae variable V783 Cygni, rather than two separate line segments as previously suspected. These new parabolic elements, JD_max = 2436394.332 + 0.62069669 + 7.5 x 10^-11 E^2, imply a gradual period increase at the rate of 0.088+-0.023 day/million years.

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