The peculiar light variations of the central star of planetary nebula V651 Mon.

Details The peculiar light variations of the central star of planetary nebula V651 Mon. The peculiar light variations of the central star of planetary nebula V651 Mon.

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993acasn..34..221h&link_type=abstract

Acta Astron. Sin., Vol. 34, No. 2, p. 221 - 224

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Scientific paper

The author presents photographic photometry of V651 Mon during 1988 - 1989. The observations and the parameters of the light curves of V651 Mon are given. From the observations it is found that the brightness variations of V651 Mon changed substantially from 1987 to 1988. It is reasonable to think that the binary central star of the planetary nebula V651 Mon might undergo another mass ejection from the subdwarf O component during 1987 - 1988.

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