Photometric characteristics of the Be stars: almost twenty years of UBV monitoring at the Hvar observatory
1994 ◽
Vol 162
◽
pp. 301-302
Keyword(s):
Be Stars
◽
Since their discovery (by Father Secchi in 1866) until the end of sixties, Be stars were not a subject of any systematic studies of their possible light and colour variations. Already at that time, the astronomical literature contained ample evidence showing that a number of Be stars were light variables. However, almost all such findings resulted as by-products of studies of different or wider groups of objects. Feinstein (1968) was probably the first who pointed out explicitly that many Be stars are light variables. A pioneering study which was aimed at the detection of light variations of a large group of Be stars by means of differential photoelectric photometry was carried out by Haupt & Schroll (1974).
Keyword(s):
2001 ◽
Vol 1
(5-6)
◽
pp. 233-243
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Keyword(s):
1994 ◽
Vol 162
◽
pp. 241-253