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- W1653993988 abstract "A new investigation of the behaviour of the star 53Per was performed. New photometric observations allow to confirmtwodominantperiodsp1=2.16d,p2=1.67d.Athirdone p3= 3.64d is detected. These long period variations are present in our radial velocities data and in old equivalent width data. The amplitude of the p1 = 2.16d period increases from 1977 to 1991, while the amplitude of the 1.67d period remains con- stant. Considering the observational characteristics of the star since 1997, 53Per clearly belongs to the Slowly Pulsating B stars group as defined by Waelkens (1991) and North & Paltani (1994)." @default.
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- W1653993988 date "1998-03-01" @default.
- W1653993988 modified "2023-09-27" @default.
- W1653993988 title "53 Persei: a slowly pulsating B star" @default.
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