The 340-d period in beta Lyrae

Details The 340-d period in beta Lyrae The 340-d period in beta Lyrae

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997mnras.284..148p&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 284, Issue 1, pp. 148-150.

Astronomy and Astrophysics

Astronomy

3

Techniques: Photometric, Binaries: Eclipsing, Binaries: General, Stars: Individual: Beta Lyrae

Scientific paper

The 340-d periodicity in the orbital residuals of the visual estimates
of beta Lyrae by M. Luizet, between 1898 and 1916, is shown not to be an
artefact, thus suggesting interference between this periodicity and the
practically commensurable period of 283.4d and, in conjunction with
recent photometry, allowing much greater cycle counts.

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