Changes in the periods of double exploding stars

Details Changes in the periods of double exploding stars Changes in the periods of double exploding stars

Dec 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975poast..23..281k&link_type=abstract

Postepy Astronomii, vol. 23, Oct.-Dec. 1975, p. 281-288. In Polish.

Astronomy and Astrophysics

Astronomy

Binary Stars, Novae, Variable Stars, Astronomical Catalogs, Graphs (Charts), Periodic Variations

Scientific paper

Concise literature survey of data reported on double exploding stars. Tabular and graphical data and comments are provided on research done on: T Aur, Z Cha, EM Cyg, U Gem, DQ Her, EX Hya, V Sge, VZ Scl, UX UMa, RW Tri. The period variations are generally interpreted as responses to: (1) mass exchange between the members of the binary system; (2) mass loss by the system as an entity; (3) changes in the orbital momentum caused by exchange of orbital momentum and rotational momenta of the components and the disk. The theory behind (3) rests on uncovering eventual periodic changes in the period of the binary system.

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