A possible second period for HD 200925 = V 1719 CYG

Details A possible second period for HD 200925 = V 1719 CYG A possible second period for HD 200925 = V 1719 CYG

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...158..389m&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 158, no. 1-2, April 1986, p. 389-391.

Astronomy and Astrophysics

Astrophysics

6

Power Spectra, Spectrum Analysis, Stellar Oscillations, Variable Stars, Light Curve, Stellar Spectrophotometry

Scientific paper

All the available photometry of HD 200925 ≡ V1719 Cyg is discussed
here and a possible second period P2 = 0.2138d is derived. In
this case the star could be a double mode pulsator in the first and
second radial overtones.

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