An estimate of the upper limit to the mass of possible secondary components of CP stars

Details An estimate of the upper limit to the mass of possible secondary components of CP stars An estimate of the upper limit to the mass of possible secondary components of CP stars

May 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pazh...13..214k&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 13, no. 3, 1987, p. 214-217. In Russian. In Russian. In Russian.

Statistics

Computation

Binary Stars, Computational Astrophysics, Peculiar Stars, Stellar Composition, Stellar Mass, Neutron Stars, Orbital Elements, Stellar Evolution, White Dwarf Stars

Scientific paper

The phase variations of the line profiles of five chemically peculiar stars are investigated using the inverse problem method. The results indicate that the profiles have not been perturbed by orbital motion which occurs with a secondary-component mass of greater than 0.3 solar mass. It is noted that the more massive component can transform into either a neutron star or a white dwarf.

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