The effects of binarity in driving CP phenomena
| dc.creator | Budaj, J. | |
| dc.date | 1998-05-06 | |
| dc.date.accessioned | 2026-07-07T02:26:48Z | |
| dc.date.available | 2026-07-07T02:26:48Z | |
| dc.description | A lot of evidence has recently accumulated that physical characteristics of CP stars (delta m_1, Ca/Fe ratio, Li abundance, distribution of orbital periods, vsini, Delta (V1-G), magnetic field) depend on orbital period or eccentricity. Consequently, the "tidal mixing + stabilization" hypothesis has been formulated to account for such features and the "binarity x magnetism" hypothesis of Abt & Snowden (1973) was reanalyzed. We conclude that all mentioned characteristics and properties of CP stars, including even CP star magnetism, may be affected or governed by binarity. | |
| dc.description | 5 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/9805055 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9805055 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/12425 | |
| dc.subject | Astrophysics | |
| dc.title | The effects of binarity in driving CP phenomena | |
| dc.type | text |