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- W1489930510 abstract "Abstract From 1978 December to 1979 May, we made spectrographic observations of φPer, ζTau and κDra using our 60 90 Schmidt cassegrain grating spectrograph. Values of electron density, rotational speed and V R variation have been obtained and a comparison between ζTau and the supergiant βOri carried out. We found that, over our observed period, θPer showed clear shell activities, ζTau was in a relatively calm phase, its shell slowly expanding, while κDra had all the signs of a “classical” Be star." @default.
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- W1489930510 date "1981-09-01" @default.
- W1489930510 modified "2023-09-26" @default.
- W1489930510 title "Photometric studies of three Be stars" @default.
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- W1489930510 doi "https://doi.org/10.1016/0275-1062(81)90058-8" @default.
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