The Variable Star V4374 Sgr

Details The Variable Star V4374 Sgr The Variable Star V4374 Sgr

Mar 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000soust..38..223a&link_type=abstract

Southern Stars, vol. 38, issue 7, p.223-230

Physics

Scientific paper

Photometric data on the variable star V4374 Sgr, obtained in 1992 at the Mt John University Observatory and the former Black Birch Outstation of Carter Observatory, have been analysed. It is found that combination of observed effects can best be modelled by a pair of sun-like rapidly rotating stars in a non-eclipsing configuration. The major photometric effects are then due to the effects of maculation. Grazing eclipses cannot be ruled out, however.

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