Oct 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000ibvs.4963....1z&link_type=abstract
Information Bulletin on Variable Stars, 4963, 1.
Physics
Variable Stars, Photometry
Scientific paper
New photoelectric photometry of P Cygni made between 1987 and 1993 is
presented. The cycle lengths derived from the light curve are
approximately 27 and 220 days, respectively. The approx. 220 day period
implies a connection with the observed shell ejections which has an
ejection period of about 200 days.
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