Grids of stellar models including second harmonic and colors: solar composition (Z=0.0172, X=0.7024)

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dc.contributor.authorYildiz, Mutlu
dc.date.accessioned2019-10-27T22:59:00Z
dc.date.available2019-10-27T22:59:00Z
dc.date.issued2015
dc.departmentEge Üniversitesien_US
dc.description.abstractGrids of stellar evolution are required in many fields of astronomy/astrophysics, such as planet hosting stars, binaries, clusters, chemically peculiar stars, etc. In this study, a grid of stellar evolution models with updated ingredients and recently determined solar abundances is presented. The solar values for the initial abundances of hydrogen, heavy elements and mixing-length parameter are 0.0172, 0.7024 and 1.98, respectively. The mass step is small enough (0.01 M-circle dot) that interpolation for a given star mass is not required. The range of stellar mass is 0.74 to 10.00 M-circle dot. We present results in different forms of tables for easy and general application. The second stellar harmonic, required for analysis of apsidal motion of eclipsing binaries, is also listed. We also construct rotating models to determine the effect of rotation on stellar structure and derive fitting formulae for luminosity, radius and the second harmonic as a function of rotational parameter. We also compute and list colors and bolometric corrections of models required for transformation between theoretical and observational results. The results are tested for the Sun, the Hyades cluster, the slowly rotating chemically peculiar Am stars and eclipsing binaries with apsidal motion. The theoretical and observational results along isochrones are in good agreement. The grids are also applicable to rotating stars provided that equatorial velocity is given.en_US
dc.description.sponsorshipScientific and Technological Research Council of TurkeyTurkiye Bilimsel ve Teknolojik Arastirma Kurumu (TUBITAK) [TUBITAK 112T989]en_US
dc.description.sponsorshipCenk Kayhan and Ilknur Gezer are acknowledged for checking the language of the manuscript. This work is supported by the Scientific and Technological Research Council of Turkey (TUBITAK 112T989).en_US
dc.identifier.doi10.1088/1674-4527/15/12/012
dc.identifier.endpage2262en_US
dc.identifier.issn1674-4527
dc.identifier.issue12en_US
dc.identifier.startpage2244en_US
dc.identifier.urihttps://doi.org/10.1088/1674-4527/15/12/012
dc.identifier.urihttps://hdl.handle.net/11454/51698
dc.identifier.volume15en_US
dc.identifier.wosWOS:000367563300012en_US
dc.identifier.wosqualityQ3en_US
dc.indekslendigikaynakWeb of Scienceen_US
dc.language.isoenen_US
dc.publisherNatl Astronomical Observatories, Chin Acad Sciencesen_US
dc.relation.ispartofResearch in Astronomy and Astrophysicsen_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanıen_US
dc.rightsinfo:eu-repo/semantics/closedAccessen_US
dc.subjectstars: interioren_US
dc.subjectstars: evolutionen_US
dc.subjectbinaries: eclipsingen_US
dc.subjectstars: chemically peculiaren_US
dc.titleGrids of stellar models including second harmonic and colors: solar composition (Z=0.0172, X=0.7024)en_US
dc.typeArticleen_US

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