Mixing-length parameter from binaries and clusters
| dc.contributor.author | Yildiz, Mutlu | |
| dc.contributor.editor | Deng, L | |
| dc.contributor.editor | Chan, KL | |
| dc.date.accessioned | 2019-10-27T19:56:09Z | |
| dc.date.available | 2019-10-27T19:56:09Z | |
| dc.date.issued | 2008 | |
| dc.department | Ege Üniversitesi | en_US |
| dc.description | 252nd Symposium of the International-Astronomical-Union -- APR 06-11, 2008 -- Sanya, PEOPLES R CHINA | en_US |
| dc.description.abstract | Mixing length parameter of the mixing length theory is a free parameter and used to calibrate radii of late-type stars. From the Hyades cluster and the alpha Centauri system, we find that the parameter depends on the stellar mass and some other properties of stars. Considering some other systems, we describe how the parameter depends on stellar parameters. | en_US |
| dc.description.sponsorship | Int Astron Union, Natl Nat Sci Fdn China, Chinese Acad Sci, Natl Astron Observatories | en_US |
| dc.identifier.doi | 10.1017/S1743921308022734 | |
| dc.identifier.endpage | 187 | en_US |
| dc.identifier.isbn | 978-0-521-88983-4 | |
| dc.identifier.issn | 1743-9213 | |
| dc.identifier.issn | 1743-9213 | en_US |
| dc.identifier.issue | 252 | en_US |
| dc.identifier.scopusquality | Q4 | en_US |
| dc.identifier.startpage | 183 | en_US |
| dc.identifier.uri | https://doi.org/10.1017/S1743921308022734 | |
| dc.identifier.uri | https://hdl.handle.net/11454/40782 | |
| dc.identifier.wos | WOS:000263138600033 | en_US |
| dc.identifier.wosquality | N/A | en_US |
| dc.indekslendigikaynak | Scopus | en_US |
| dc.indekslendigikaynak | Web of Science | en_US |
| dc.language.iso | en | en_US |
| dc.publisher | Cambridge Univ Press | en_US |
| dc.relation.ispartof | Art of Modelling Stars in the 21St Century | en_US |
| dc.relation.ispartofseries | IAU Symposium Proceedings Series | |
| dc.relation.publicationcategory | Konferans Öğesi - Uluslararası - Kurum Öğretim Elemanı | en_US |
| dc.rights | info:eu-repo/semantics/openAccess | en_US |
| dc.subject | convection | en_US |
| dc.subject | stars: interiors | en_US |
| dc.subject | stars: evolution | en_US |
| dc.subject | stars: late-type | en_US |
| dc.subject | binaries: eclipsing | en_US |
| dc.subject | stars: individual (alpha Cen, FL Lyr, V442 Cyg) | en_US |
| dc.title | Mixing-length parameter from binaries and clusters | en_US |
| dc.type | Conference Object | en_US |
