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Article overview
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Magnetic Bp and Ap stars in the H-R diagram | | S. Hubrig
; P. North
; G. Mathys
; | | Date: |
6 May 1998 | | Subject: | astro-ph | | Affiliation: | Potsdam), P. North (Lausanne), G. Mathys (ESO | | 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. | | Source: | arXiv, astro-ph/9805074 | | Services: | Forum | Review | PDF | Favorites | |
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