{ "id": "0911.0749", "version": "v1", "published": "2009-11-04T08:29:14.000Z", "updated": "2009-11-04T08:29:14.000Z", "title": "Models of $μ$ Her with asteroseismic constraints", "authors": [ "W. Yang", "X. Meng" ], "comment": "14 pages and 8 figures", "categories": [ "astro-ph.SR" ], "abstract": "Using the Yale stellar evolution code, models of mu Her based on asteroseismic measurements are constructed. A $\\chi^{2}$ minimization is performed to approach the best modeling parameters which reproduce the observations within their errors. By combining all non-asteroseismic constraints with asteroseismic measurements, we find that the observational constraints favour a model with a mass of 1.00$^{+ 0.01}_{- 0.02}$ $M_{\\odot}$, an age t = 6.433 $\\pm$ 0.04 Gyr, a mixing-length parameter $\\alpha$ = 1.75 $\\pm$ 0.25, an initial hydrogen abundance $X_{i}$ = 0.605$^{+ 0.01}_{- 0.005}$ and metal abundance $Z_{i}$ = 0.0275$^{+ 0.002}_{- 0.001}$. mu Her is in post-main sequence phase of evolution. The modes of $l$ = 1 show up the characteristics of avoided crossings, which may be applied to test the internal structure of this type stars. Asteroseismic measurements can be used as a complementary constraint on the modeling parameters. The models with mass 1.00 - 1.10 $M_{\\odot}$ can reproduce the observational constraints. Existing observed data of mu Her do not rule out these models.", "revisions": [ { "version": "v1", "updated": "2009-11-04T08:29:14.000Z" } ], "analyses": { "keywords": [ "asteroseismic measurements", "yale stellar evolution code", "observational constraints favour", "post-main sequence phase", "initial hydrogen abundance" ], "tags": [ "journal article" ], "publication": { "doi": "10.1016/j.newast.2009.11.001", "journal": "New Astronomy", "year": 2010, "month": "Apr", "volume": 15, "number": 4, "pages": 367 }, "note": { "typesetting": "TeX", "pages": 14, "language": "en", "license": "arXiv", "status": "editable", "inspire": 836060, "adsabs": "2010NewA...15..367Y" } } }