New absolute magnitude calibrations for detached binaries

被引:25
作者
Bilir, S. [1 ]
Ak, T. [1 ,2 ]
Soydugan, E. [3 ]
Soydugan, F. [3 ]
Yaz, E. [1 ]
Ak, N. Filiz [3 ,4 ]
Eker, Z. [2 ,3 ]
Demircan, O.
Helvaci, M. [5 ]
机构
[1] Istanbul Univ, Fac Sci, Dept Astron & Space Sci, TR-34119 Istanbul, Turkey
[2] TUBITAK Natl Observ, TR-07058 Antalya, Turkey
[3] Canakkale Onsekiz Mart Univ, Fac Sci & Arts, Dept Phys, TR-17100 Canakkale, Turkey
[4] Erciyes Univ, Fac Sci & Arts, Dept Astron & Space Sci, TR-38039 Kayseri, Turkey
[5] Ankara Univ, Fac Sci, Dept Astron & Space Sci, TR-06100 Ankara, Turkey
关键词
stars: distances; binaries: eclipsing;
D O I
10.1002/asna.200811002
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Lutz-Kelker bias corrected absolute magnitude calibrations for the detached binary systems with main-sequence components are presented. The absolute magnitudes of the calibrator stars were derived at intrinsic colours of Johnson-Cousins and 2MASS (Two Micron All Sky Survey) photometric systems. As for the calibrator stars, 44 detached binaries were selected from the Hipparcos catalogue, which have relative observed parallax errors smaller than 15% (sigma(pi)/pi <= 0.15). The calibration equations which provide the corrected absolute magnitude for optical and near-infrared pass bands are valid for wide ranges of colours and absolute magnitudes: -0.18 < (B - V)(0) < 0.91, -1.6 < M-V < 5.5 and -0.15 < (J - H)(0) < 0.50, -0-02 < (H - K-s)(0) < 0. 13, 0 < M-J < 4, respectively. The distances computed using the luminosity-colours (LCs) relation with optical (B V) and near-infrared (J H K-s) observations were compared to the distances found from various other methods. The results show that new absolute magnitude calibrations of this study can be used as a convenient statistical tool to estimate the true distances of detached binaries out of Hipparcos' distance limit. (C) 2008 WILEY-VCH Verlag GmbH & Co. KGaA. Weinheim
引用
收藏
页码:835 / 844
页数:10
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