dc.contributor.author | Napiwotzki, R. | |
dc.contributor.author | Rieschick, A. | |
dc.contributor.author | Blocker, T. | |
dc.contributor.author | Schonberner, D. | |
dc.contributor.author | Wenske, V. | |
dc.date.accessioned | 2008-01-27T15:29:44Z | |
dc.date.available | 2008-01-27T15:29:44Z | |
dc.date.issued | 1993 | |
dc.identifier.citation | Napiwotzki , 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.isbn | 0-937707-59-7 | |
dc.identifier.other | dspace: 2299/1416 | |
dc.identifier.uri | http://hdl.handle.net/2299/1416 | |
dc.description | Original paper can be found at: http://www.astrosociety.org/pubs/cs/confseries.html#2--Copyright Astronomical Society of the Pacific | |
dc.description.abstract | For 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.format.extent | 276165 | |
dc.language.iso | eng | |
dc.publisher | Astronomical Society of the Pacific | |
dc.relation.ispartof | In: Procs Inside the Stars, IAU Colloquium 137 | |
dc.title | Convective overshooting and the observed width of the main-sequence band | en |
dc.contributor.institution | School of Physics, Astronomy and Mathematics | |
dc.contributor.institution | School of Physics, Engineering & Computer Science | |
dc.contributor.institution | Department of Physics, Astronomy and Mathematics | |
dc.contributor.institution | Centre for Astrophysics Research (CAR) | |
rioxxterms.type | Other | |
herts.preservation.rarelyaccessed | true | |