Eclipsing variable stars in neighbouring galaxies. III. Discussion of the light curve of V 31 in IC 1613.

Details Eclipsing variable stars in neighbouring galaxies. III. Discussion of the light curve of V 31 in IC 1613. Eclipsing variable stars in neighbouring galaxies. III. Discussion of the light curve of V 31 in IC 1613.

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986geoce..15.....g&link_type=abstract

GEOS Circular on Eclipsing Binaries, No. EB 15, 6 p. (1986)

Computer Science

Eclipsing Binaries:Galaxies, Light Curves

Scientific paper

The light curve of the only eclipsing variable so far discovered in IC 1613, a galaxy belonging to the Local Group, is discussed in this paper by applying a method of analysis in the frequency domain in order to obtain the photometric orbital elements. The solution, which appears to be well determined, shows that V 31 is an Algol-type system in which the larger component is probably more evolved than its companion. However, owing to the lack of spectroscopic data, it does not seem proper to venture any hypothesis on the present evolutionary stage of the system.

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