GSC3658-0076: A Binary System at the Beginning of Mass Transfer

Details GSC3658-0076: A Binary System at the Beginning of Mass Transfer GSC3658-0076: A Binary System at the Beginning of Mass Transfer

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ap%26ss.299..329z&link_type=abstract

Astrophysics and Space Science, Volume 299, Issue 4, pp.329-341

Astronomy and Astrophysics

Astrophysics

1

Stars, Binaries, Close, Stars, Individual (Gsc3658-0076)

Scientific paper

Photometric data of the new discovered binary GSC3658-0076 observed by [González-Rojas et al.: 2003, IBVS, No. 5437.] were analyzed using the latest Wilson-Devinney code. The system turns out to be a detached binary system with the primary component almost filling its Roche lobe, while the secondary one is detached from the critical Roche lobe. According to the mass-radius relation of unevolved (ZAMS) detached binaries given by [Demircan and Kahraman: 1991, Ap&SS 181, 313.], the primary component is more evolved. These properties reveal that GSC3658-0076 may be at the beginning of the mass transfer phase and may evolve from the present detached system into a contact binary or be in the broken-contact phase predicted by TRO theory.

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