HOT EMISSION-LINE STARS
AFTER 134 YEARS OF STUDY
Petr Harmanec1,2
1
Astronomical Institute of the Charles University,
V Holesovickach 2, CZ-180 00 Praha 8, Czech Republic
2
Astronomical Institute of the Academy of Sciences,
CZ-251 65 Ondrejov, Czech Republic
A brief review of current problems in the research of hot
emission-line stars is presented. Special attention is paid to
problems of reliable determination of basic physical properties of
underlying stars and to possible role of duplicity in the whole
phenomenon. A preliminary catalogue of OBA emission-line stars in
binaries is also included.
To appear in: 2000, ``Interacting Astronomers: A Symposium on
Mirek Plavec's Favourite Stars'', Publications of the Astronomical
Institute of the Academy of Sciences of the Czech Republic No. 89,
Ed. by P. Harmanec, P. Hadrava and I. Hubeny, pp. 9-22
Preprints from
hec@sunstel.asu.cas.cz
or by anonymous ftp to
ftp://astro.mff.cuni.cz/HEC/PAPERS/hec2000.ps
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