The calibration of the RGB tip as a standard candle - Extension to near infrared colors and higher metallicity

被引:122
作者
Bellazzini, M
Ferraro, FR
Sollima, A
Pancino, E
Origlia, L
机构
[1] Osservatorio Astron Bologna, INAF, I-40127 Bologna, Italy
[2] Univ Bologna, Dipartimento Astron, I-40127 Bologna, Italy
关键词
distance scale; globular clusters : individual : NGC 5139; NGC; 104; stars : Population II; Magellanic Clouds;
D O I
10.1051/0004-6361:20035910
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
New empirical calibrations of the Red Giant Branch Tip in the I, J, H and K bands based on two fundamental pillars, namely omega Centauri and 47 Tucanae, have been obtained by using a large optical and near infrared photometric database. Our best estimates give M-I(TRGB)=-4.05+/-0.12, M-J(TRGB)=-5.20+/-0.16, M-H(TRGB)=-5.94+/-0.18 and M-K(TRGB)=-6.04+/-0.16 at [M/H] 1.5 (omega Cen) and M-I(TRGB)=-3.91+/-0.13, M-J(TRGB)=-5.47+/-0.25, M-H(TRGB)=-6.35+/-0.30 and M-K(TRGB)=-6.56+/-0.20 at [M/H]similar or equal to -0.6 (47 Tuc). With these new empirical calibrations we also provide robust relations of the TRGB magnitude in the I, J, H, and K bands as a function of the global metallicity. It has also been shown that our calibrations self-consistently provide a distance modulus of the Large Magellanic Cloud in good agreement with the standard value ((m-M)(0) similar or equal to 18.50)).
引用
收藏
页码:199 / 211
页数:13
相关论文
共 82 条
[1]  
ALVES D, 2003, IN PRESS LECT NOTES
[2]   A review of the distance and structure of the Large Magellanic Cloud [J].
Alves, DR .
NEW ASTRONOMY REVIEWS, 2004, 48 (09) :659-665
[3]   Variations in star formation history and the red giant branch tip [J].
Barker, MK ;
Sarajedini, A ;
Harris, J .
ASTROPHYSICAL JOURNAL, 2004, 606 (02) :869-893
[4]   A step toward the calibration of the red giant branch tip as a standard candle [J].
Bellazzini, M ;
Ferraro, FR ;
Pancino, E .
ASTROPHYSICAL JOURNAL, 2001, 556 (02) :635-640
[5]   The Draco and Ursa minor dwarf spheroidal galaxies: A comparative study [J].
Bellazzini, M ;
Ferraro, FR ;
Origlia, L ;
Pancino, E ;
Monaco, L ;
Oliva, E .
ASTRONOMICAL JOURNAL, 2002, 124 (06) :3222-3240
[6]   Automatic abundance analysis of high resolution spectra [J].
Bonifacio, P ;
Caffau, E .
ASTRONOMY & ASTROPHYSICS, 2003, 399 (03) :1183-1192
[7]   High-resolution CCD spectra of stars in globular clusters .9. The ''young'' clusters Ruprecht 106 and Pal 12 [J].
Brown, JA ;
Wallerstein, G ;
Zucker, D .
ASTRONOMICAL JOURNAL, 1997, 114 (01) :180-188
[8]   Ultraviolet properties of primeval galaxies: Theoretical models from stellar population synthesis [J].
Buzzoni, A .
ASTRONOMICAL JOURNAL, 2002, 123 (03) :1188-1199
[10]  
Cacciari C, 1999, ASTR SOC P, V167, P140