The pulsation period of the Beta Cephei-star Nu Centauri

Details The pulsation period of the Beta Cephei-star Nu Centauri The pulsation period of the Beta Cephei-star Nu Centauri

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ap%26ss.192...79a&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 192, no. 1, June 1992, p. 79-82.

Astronomy and Astrophysics

Astrophysics

3

Binary Stars, Radial Velocity, Stellar Orbits, Ephemeris Time, Periodic Variations

Scientific paper

An attempt is made to refine the pulsation period of the Beta Cephei
star Nu Centauri by observing the star continuously over a pulsation
cycle in different seasons. A new ephemeris with a pulsation period of
0.169401 d is derived by combining data for three seasons over a period
of three years. The new estimate fits well in phase with earlier data.

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