Constancy of period in TX Ceti

Details Constancy of period in TX Ceti Constancy of period in TX Ceti

Apr 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.166..205s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 166, no. 2, April 1990, p. 205-210.

Astronomy and Astrophysics

Astrophysics

Eclipsing Binary Stars, Orbital Elements, Stellar Motions, Astronomical Photometry, Tables (Data), Three Body Problem

Scientific paper

A slightly improved period (P = 0.7408401 d) of the eclipsing binary system TX Ceti is given which is based on all available times of minima. The O-C diagrams based on the period given in PPEN (1980) and based on the new period are given. The period of TX Ceti shows fair constancy between the time interval 1928 to 1988. The present O-C diagrams do not confirm either the presence of a third body or the presence of mass transfer.

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