High-precision effective temperatures of 161 FGK supergiants from line-depth ratios

被引:102
作者
Kovtyukh, V. V. [1 ]
机构
[1] Odessa Astron Observ, UA-65014 Odessa, Ukraine
关键词
star : fundamental parameters; supergiants; Cepheids;
D O I
10.1111/j.1365-2966.2007.11804.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Precise effective temperatures (T-eff) are determined for 161 FGK supergiants using method of line-depth ratios. We obtain a set of 131 relations for temperatures of supergiants as a function of line depths. These relations have been calibrated against previously published accurate temperature estimates. The application range of the method is 3600-7800 K (F0I-K5I). The internal error of a single calibration is less than 110 K, while combination of all calibrations reduces uncertainty to only 5-30 K (standard error). The error in the zero-point is estimated to be less than 100-200 K. A significant advantage of the line ratio method is its independence of the interstellar reddening, and only modest sensitivity to abundance, macroturbulence, rotation and other factors.
引用
收藏
页码:617 / 624
页数:8
相关论文
共 34 条
[1]  
Alfaro HB, 1997, PUBL ASTRON SOC PAC, V109, P958, DOI 10.1086/133967
[2]   Phase-dependent variation of the fundamental parameters of Cepheids. III. Periods between 3 and 6 days [J].
Andrievsky, SM ;
Luck, RE ;
Kovtyukh, VV .
ASTRONOMICAL JOURNAL, 2005, 130 (04) :1880-1889
[3]  
BAGNULO S, 2003, ESO MESSENGER, V114, P10
[4]  
Bersier D, 1996, ASTRON ASTROPHYS, V308, P514
[5]  
Bessell MS, 1998, ASTRON ASTROPHYS, V333, P231
[6]   Determination of the temperatures of selected ISO flux calibration stars using the Infrared Flux Method [J].
Blackwell, DE ;
Lynas-Gray, AE .
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES, 1998, 129 (03) :505-515
[7]   Catalogue of [Fe/H] determinations for FGK stars: 2001 edition [J].
de Strobel, GC ;
Soubiran, C ;
Ralite, N .
ASTRONOMY & ASTROPHYSICS, 2001, 373 (01) :159-163
[8]   Transformations from theoretical Hertzsprung-Russell diagrams to color-magnitude diagrams: Effective temperatures, B-V colors, and bolometric corrections [J].
Flower, PJ .
ASTROPHYSICAL JOURNAL, 1996, 469 (01) :355-365
[9]   Chemical abundances of Galactic cepheid variables that calibrate the P-L relation [J].
Fry, AM ;
Carney, BW .
ASTRONOMICAL JOURNAL, 1997, 113 (03) :1073-1087
[10]  
GALAZUTDINOV GA, 1992, PREPRINT SAO RAS, V92, P28