A new absolute magnitude calibration with 2MASS for cataclysmic variables

被引:30
作者
Ak, T. [1 ]
Bilir, S. [1 ]
Ak, S. [1 ]
Retter, A. [1 ]
机构
[1] Istanbul Univ, Fac Sci, Dept Astron & Space Sci, TR-34119 Istanbul, Turkey
基金
美国国家科学基金会; 美国国家航空航天局;
关键词
cataclysmic binaries; distances; parallaxes;
D O I
10.1016/j.newast.2007.01.002
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Using reliable trigonometric measurements, we find that the absolute magnitude of cataclysmic variables depends on the orbital period and de-reddened (J - H)(0) and (H - K-s)(0) colours of 2MASS (Two Micron All Sky Survey) photometric system. The calibration equation covers the ranges 0.032(d) < P-orb <= 0.454(d) , -0.08 < (J - H)(0) <= 1.54, -0.03 < (H - K-s)(0) <= 0.56 and 2.0 <= M-J < 11.7; It is based on trigonometric parallaxes with relative errors of (sigma(pi)/pi) <= 0.4. By using the period-1 uminosity-colours (PLCs) relation, we estimated the distances of cataclysmic variables with orbital periods and 2MASS observations and compared them with distances found from other methods. We suggest that the PLCs relation can be a useful statistical tool to estimate the distances of cataclysmic variables. (C) 2007 Elsevier B.V. All rights reserved.
引用
收藏
页码:446 / 453
页数:8
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