The Long Period Variations of UZ Persei

Details The Long Period Variations of UZ Persei The Long Period Variations of UZ Persei

Jul 1929

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1929natur.124...93z&link_type=abstract

Nature, Volume 124, Issue 3116, pp. 93-94 (1929).

Physics

Scientific paper

IN Harvard College Observatory Bulletin, No. 867, Feb. 1, 1929, there is a note by B. P. Gerasimovič on ``UZ Persei, a Variable of Unusually Long Period''. The author found that the brightness of this variable star has two oscillations-short and long-with periods of about 90 and 907 days respectively. It is known that such oscillations are typical for µ Cephei.

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