CAOSP abstracts, Volume: 27, No.: 3, year: 1998
- Author(s): HUBRIG, S.; P. NORTH, P.; MATHYS, G.
- Journal: Contributions of the Astronomical Observatory Skalnate Pleso,
vol. 27, no. 3, p. 249-251.
- Date: 04/1998
- Title: Magnetic Bp and Ap stars in the H-R diagram
- Keyword(s): H-R DIAGRAM, MAGNETIC STARS
- Pages: 249 -- 251
Abstract:
The positions in the H-R diagram of strongly magnetic Ap and Bp
stars are compared with those of normal main sequence stars of types
B7 to F2, with a view to investigating possible differences in evolutionary
status between magnetic and non-magnetic stars. The normal B7-F2 stars fill
the whole width of the main sequence band with some concentration towards
the ZAMS, whereas the magnetic stars are only rarely found close to either
the zero-age or terminal-age sequences.
Full text version of this article in
PostScript
(600dpi) format compressed by gzip; or in
PDF.
