Eclipsing variable stars in neighbouring galaxies. II. Discussion of the light curve of V 55 in NGC 2403.

Details Eclipsing variable stars in neighbouring galaxies. II. Discussion of the light curve of V 55 in NGC 2403. Eclipsing variable stars in neighbouring galaxies. II. Discussion of the light curve of V 55 in NGC 2403.

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986geoce..14.....g&link_type=abstract

GEOS Circular on Eclipsing Binaries, No. EB 14, 8 p. (1986)

Other

Eclipsing Binaries:Light Curves, Spiral Galaxies

Scientific paper

The light curve of the eclipsing variable V 55 in the spiral galaxy NGC 2403 is discussed by means of an analysis in the frequency domain in order to obtain photometric orbital elements. The solution of the orbit shows that V 55 is a detached system whose components, differing very little from each other, should belong to the earlier spectral classes. The binary system discussed here appears to be the remotest system so far discovered.

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