Effective temperatures of CP stars
| dc.creator | Sokolov, N. A. | |
| dc.date | 1998-05-12 | |
| dc.date.accessioned | 2026-07-07T02:26:53Z | |
| dc.date.available | 2026-07-07T02:26:53Z | |
| dc.description | A new method of T_eff determination for CP stars is proposed. The method is based on the fact that the slope of the energy distribution in the Balmer continuum near the Balmer jump is identical for "normal" main sequence stars and for CP stars with the same T_eff. It is shown that the T_eff of CP stars derived by this method are in good agreement with those derived by other methods. | |
| dc.description | 3 pages, 1 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/9805149 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9805149 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/12463 | |
| dc.subject | Astrophysics | |
| dc.title | Effective temperatures of CP stars | |
| dc.type | text |