Light variability of Nova Delphini 1967 in 1977 and 1979

Details Light variability of Nova Delphini 1967 in 1977 and 1979 Light variability of Nova Delphini 1967 in 1977 and 1979

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....92..200k&link_type=abstract

Astronomy and Astrophysics, vol. 92, no. 1-2, Dec. 1980, p. 200-203.

Astronomy and Astrophysics

Astrophysics

12

Light Curve, Novae, Stellar Spectrophotometry, Ubv Spectra, Binary Stars, Electrophotometry, Periodic Variations

Scientific paper

Photoelectric UBV photometry of N Del 1967 indicates a short-period
sinusoidal light variability with P = 0.1775d and with a V-amplitude of
0.16 (in 1977) and 0.10 mag (in 1979). The photometric period appears to
be identical with the spectroscopic period which probably reflects the
orbital motion of the binary.

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