Mira stars - II: R Cam, R Cas, W Cas, S Cep, T Cep, U CYG and S Del

Details Mira stars - II: R Cam, R Cas, W Cas, S Cep, T Cep, U CYG and S Del Mira stars - II: R Cam, R Cas, W Cas, S Cep, T Cep, U CYG and S Del

Jun 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989jbaa...99..121i&link_type=abstract

Journal of the British Astronomical Association, vol.99, no.3, p.121-129

Astronomy and Astrophysics

Astronomy

12

Scientific paper

Some 52,000 visual observations of seven Mira stars, observed for between 10 and 74 years, are analysed, and the results are compared with catalogue data. A number of interesting correlations are found among features in the light curves. S Cep and U Cyg are found to vary slowly in their mean brightness, while R Cam, T Cep and U Cyg vary slowly in amplitude. The mean period of T Cep is confirmed to show evidence of variation, but those of R Cam and U Cyg are not found to vary.

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