Constraints on cataclysmic variable evolution from the triple system 4 Draconis

Details Constraints on cataclysmic variable evolution from the triple system 4 Draconis Constraints on cataclysmic variable evolution from the triple system 4 Draconis

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...345..489e&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 345, Oct. 1, 1989, p. 489-491. Research supported by SERC.

Astronomy and Astrophysics

Astrophysics

8

Binary Stars, Cataclysmic Variables, Dwarf Novae, Stellar Evolution, Triple Stars, Giant Stars, Mass Distribution, Stellar Mass Accretion

Scientific paper

The paper considers the evolution of the triple system 4 Dra, which now
comprises a cataclysmic variable in a P of about 1700d orbit with an M
giant. It is found that the requirement of dynamical stability imposes
significant restrictions on the precursor system of the CV.

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