Towards 21st century stellar models: Star clusters, supercomputing and asteroseismology
AuthorCampbell, S. W.
Constantino, T. N.
De Silva, G. M.
Arnett, W. D.
Lattanzio, J. C.
MacLean, B. T.
AffiliationUniv Arizona, Steward Observ
MetadataShow full item record
PublisherWILEY-V C H VERLAG GMBH
CitationTowards 21st century stellar models: Star clusters, supercomputing and asteroseismology 2016, 337 (8-9):788 Astronomische Nachrichten
Rights© 2016 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim
Collection InformationThis item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at email@example.com.
AbstractStellar models provide a vital basis for many aspects of astronomy and astrophysics. Recent advances in observational astronomy - through asteroseismology, precision photometry, high-resolution spectroscopy, and large-scale surveys - are placing stellar models under greater quantitative scrutiny than ever. The model limitations are being exposed and the next generation of stellar models is needed as soon as possible. The current uncertainties in the models propagate to the later phases of stellar evolution, hindering our understanding of stellar populations and chemical evolution. Here we give a brief overview of the evolution, importance, and substantial uncertainties of core helium burning stars in particular and then briefly discuss a range of methods, both theoretical and observational, that we are using to advance the modelling. (C) 2016 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim
NoteVersion of record online: 30 September 2016; 12 Month Embargo.
VersionFinal accepted manuscript