The hot side of the lithium dip - LiBeB abundances beyond the main sequence
| dc.creator | Charbonnel, Corinne | |
| dc.creator | Talon, Suzanne | |
| dc.date | 1999-09-13 | |
| dc.date.accessioned | 2026-07-07T02:33:14Z | |
| dc.date.available | 2026-07-07T02:33:14Z | |
| dc.description | We extend to the case of A and early-F type stars our study of the transport of matter and angular momentum by wind-driven meridional circulation and shear turbulence. We show that our fully consistent treatment of the same hydrodynamical processes which can account for C and N anomalies in B type stars (Talon et al. 1997) and for the shape of the hot side of the Li dip in the open clusters (Talon & Charbonnel 1998) also explains LiBeB observations in stars with Teff higher than 7000 K on the main sequence as well as in their evolved counterparts. | |
| dc.description | 10 pages, A&A, accepted | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9909209 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9909209 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/14763 | |
| dc.subject | Astrophysics | |
| dc.title | The hot side of the lithium dip - LiBeB abundances beyond the main sequence | |
| dc.type | text |