12 Bootis: the need for asteroseismic constraints

dc.creatorMiglio, A.
dc.creatorMontalban, J.
dc.creatorMaceroni, C.
dc.creatorDe Ridder, J.
dc.creatorD'Antona, F.
dc.date2006-10-16
dc.date.accessioned2026-07-07T07:26:59Z
dc.date.available2026-07-07T07:26:59Z
dc.description12 Bootis is a double-lined spectroscopic binary whose orbit has been resolved by interferometry. We present a detailed modelling of the system and show that the available observational constraints can be reproduced by models at different evolutionary stages, depending on the details of extra-mixing processes acting in the central regions. In order to discriminate among these theoretical scenarios, additional and independent observational constraints are needed: we show that these could be provided by solar-like oscillations, that are expected to be excited in both system components.
dc.description4 pages, to appear in the proceedings of SoHO18/GONG2006/HelAsI, Sheffield August 2006
dc.identifierhttps://arxiv.org/abs/astro-ph/0610471
dc.identifierhttp://arxiv.org/abs/astro-ph/0610471
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/117224
dc.subjectAstrophysics
dc.title12 Bootis: the need for asteroseismic constraints
dc.typetext

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