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dc.contributor.authorNapiwotzki, R.
dc.contributor.authorRieschick, A.
dc.contributor.authorBlocker, T.
dc.contributor.authorSchonberner, D.
dc.contributor.authorWenske, V.
dc.date.accessioned2008-01-27T15:29:44Z
dc.date.available2008-01-27T15:29:44Z
dc.date.issued1993
dc.identifier.citationNapiwotzki , R , Rieschick , A , Blocker , T , Schonberner , D & Wenske , V 1993 , Convective overshooting and the observed width of the main-sequence band . in In: Procs Inside the Stars, IAU Colloquium 137 . Astronomical Society of the Pacific , pp. 461-463 .
dc.identifier.isbn0-937707-59-7
dc.identifier.otherPURE: 142457
dc.identifier.otherPURE UUID: 0c27dc48-63f6-498d-bbb4-d700c0007e98
dc.identifier.otherdspace: 2299/1416
dc.identifier.urihttp://hdl.handle.net/2299/1416
dc.descriptionOriginal paper can be found at: http://www.astrosociety.org/pubs/cs/confseries.html#2--Copyright Astronomical Society of the Pacific
dc.description.abstractFor many years we are witnessing a lively debate on the existence and extent of convective overshooting, mainly in the cores of main-sequence stars. This is an important issue, since even a small amount of overshooting increases considerably the mass of the finally hydrogen exhausted core and lengthens the main-sequence lifetime correspondingly.en
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofIn: Procs Inside the Stars, IAU Colloquium 137
dc.rightsOpen
dc.titleConvective overshooting and the observed width of the main-sequence banden
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dcterms.dateAccepted1993
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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