Magnetic Bp and Ap stars in the H-R diagram
| dc.creator | Hubrig, S. | |
| dc.creator | North, P. | |
| dc.creator | Mathys, G. | |
| dc.date | 1998-05-06 | |
| dc.date.accessioned | 2026-07-07T02:26:51Z | |
| dc.date.available | 2026-07-07T02:26:51Z | |
| dc.description | 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. | |
| dc.description | 3 pages, no figure, to appear in: Proc. of the 26th workshop of the European Working Group on CP stars, eds. P. North, A. Schnell and J. Ziznovsky, Contrib. Astr. Obs. Skalnate Pleso Vol. 27, No 3 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9805074 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9805074 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/12441 | |
| dc.subject | Astrophysics | |
| dc.title | Magnetic Bp and Ap stars in the H-R diagram | |
| dc.type | text |