Mixed chemistry phenomenon during late stages of stellar evolution

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dc.creatorSzczerba, R.
dc.creatorSchmidt, M. R.
dc.creatorPulecka, M.
dc.date2007-04-04
dc.date.accessioned2026-07-07T07:54:31Z
dc.date.available2026-07-07T07:54:31Z
dc.descriptionWe discuss phenomenon of simultaneous presence of O- and C-based material in surroundings of evolutionary advanced stars. We concentrate on silicate carbon stars and present observations that directly confirm the binary model scenario for them. We discuss also class of C-stars with OH emission detected, to which some [WR] planetary nebulae do belong.
dc.description8 pages, 4 figures, Baltic Astronomy in press
dc.identifierhttps://arxiv.org/abs/0704.0557
dc.identifierhttp://arxiv.org/abs/0704.0557
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/126642
dc.subjectAstrophysics
dc.titleMixed chemistry phenomenon during late stages of stellar evolution
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