Presented at the 87th
Spring Meeting of the AAVSO, June 20, 1998
Abstract
Starting in October 1993,
HR 211 was observed photoelectrically in V on 76 nights over 5 years. The
complete light curve and the power spectrum reveal a period close to a month
with a possible long-term variability present. This is compared with the
Hipparcos wide-band photometry, which runs from December, 1989, to February,
1993, and consists of 68 observations. For these, a period search suggests
variability on a time-scale of about a month, with no long period apparent. An
attempt is made to explain this and other dissimilarities.