Cosmic abundances: The impact of stellar duplicity

Simple item page
dc.creatorJorissen, A.
dc.creatorVan Eck, S.
dc.date2004-10-27
dc.date.accessioned2026-07-07T02:15:31Z
dc.date.available2026-07-07T02:15:31Z
dc.descriptionThe mass-transfer scenario links chemical peculiarities with stellar duplicity for an increasing number of stellar classes (classical and dwarf barium stars, subgiant and giant CH stars, S stars without technetium, yellow symbiotic stars, WIRRING stars, Abell-35-like nuclei of planetary nebulae...). Despite these successes, the mass-transfer scenario still faces several problems: What is the mass-transfer mode? Why orbital elements of dwarf barium stars do not fully match those of the classical barium stars? What is the origin of the few non-binary stars among dwarf barium stars? The paper reviews these open questions.
dc.description14 pages, 4 figures, to appear in `Cosmic Abundances as Records of Stellar Evolution and Nucleosynthesis', edited by F.N. Bash, T.G. Barnes, ASP Conf. Ser., in press
dc.identifierhttps://arxiv.org/abs/astro-ph/0410666
dc.identifierhttp://arxiv.org/abs/astro-ph/0410666
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8440
dc.subjectAstrophysics
dc.titleCosmic abundances: The impact of stellar duplicity
dc.typetext

Files

Collections

arXiv