A Probable Periodicity in the Light Variation of the LMC Supergiant HD 33579

Details A Probable Periodicity in the Light Variation of the LMC Supergiant HD 33579 A Probable Periodicity in the Light Variation of the LMC Supergiant HD 33579

Mar 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974ibvs..877....1v&link_type=abstract

Information Bulletin on Variable Stars, 877, 1.

Physics

6

Scientific paper

Photometry of the brightest supergiant of the LMC HD 33579 in 1971,
1972, 1973 and 1974 shows evidence for a periodicity of around 90 days.
The nature is probably pulsation.

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