{ "id": "1509.07873", "version": "v1", "published": "2015-09-25T20:04:47.000Z", "updated": "2015-09-25T20:04:47.000Z", "title": "Absolute dimensions of the metallic-line eclipsing binary V501 Monocerotis", "authors": [ "Guillermo Torres", "Claud H. Sandberg Lacy", "Kresimir Pavlovski", "Francis C. Fekel", "Matthew W. Muterspaugh" ], "comment": "11 pages in emulateapj format, including 8 tables and 11 figures. Accepted for publication in The Astronomical Journal", "categories": [ "astro-ph.SR" ], "abstract": "We report extensive high-resolution spectroscopic observations and V-band differential photometry of the slightly eccentric 7.02-day detached eclipsing binary V501 Mon (A6m+F0), which we use to determine its absolute dimensions to high precision (0.3% for the masses and 1.8% for the radii, or better). The absolute masses, radii, and temperatures are M(A) = 1.6455 +/- 0.0043 M(Sun), R(A) = 1.888 +/- 0.029 R(Sun), and T(A) = 7510 +/- 100 K for the primary, and M(B) = 1.4588 +/- 0.0025 M(Sun), R(B) = 1.592 +/- 0.028 R(Sun), and T(B) = 7000 +/- 90 K for the secondary. Apsidal motion has been detected, to which General Relativity contributes approximately 70%. The primary star is found to be a metallic-line A star. A detailed chemical analysis of the disentangled spectra yields abundances for more than a dozen elements in each star. Based on the secondary, the system metallicity is near solar: [Fe/H] = +0.01 +/- 0.06. Lithium is detected in the secondary but not in the primary. A comparison with current stellar evolution models shows a good match to the measured properties at an age of about 1.1 Gyr.", "revisions": [ { "version": "v1", "updated": "2015-09-25T20:04:47.000Z" } ], "analyses": { "keywords": [ "metallic-line eclipsing binary v501 monocerotis", "absolute dimensions", "extensive high-resolution spectroscopic observations" ], "note": { "typesetting": "TeX", "pages": 11, "language": "en", "license": "arXiv", "status": "editable" } } }