Astronomy and Astrophysics – Astrophysics
Scientific paper
Mar 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26as...72..505j&link_type=abstract
Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 72, no. 3, March 1988, p. 505-513.
Astronomy and Astrophysics
Astrophysics
28
A Stars, Astronomical Photography, Shell Stars, Stellar Spectra, Balmer Series, Classifications, Stellar Color, Stellar Rotation
Scientific paper
A total of 28 northern Ae and A-type shell stars were observed in the photographic spectral region. A regular pattern of line behavior with spectral type was found, which in part prolongs the behavior of Be stars toward cooler stars, although a discontinuity seems present around A0. A survey of other data concerning colors, rotation, variability, etc., is also presented. Photometrically the stars simulate the behavior of higher-luminosity objects. A large proportion of shells seems to be variable. The attempt to detect new shell stars among 13 stars known to be rapid rotators with normal spectra failed, however.
Andrillat Yvette
Jaschek Carlos
Jaschek Mercedes
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