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Astron. Astrophys. 337, 321 (1998)

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Model atmospheres broad-band colors, bolometric corrections and temperature calibrations for O-M stars

M.S. Bessell 1, F. Castelli 2 and B. Plez 3, 4

1 Mount Stromlo and Siding Spring Observatories, Institute of Advanced Studies, The Australian National University,
Weston Creek P.O., ACT 2611, Australia
2 CNR-Gruppo Nazionale Astronomia and Osservatorio Astronomico di Trieste, Via G.B. Tiepolo 11, I-34131 Trieste, Italy
3 Astronomiska Observatoriet, Box 515, S-75120 Uppsala, Sweden
4 Atomspektroskopi, Fysiska Institution, Box 118, S-22100 Lund, Sweden

Astron. Astrophys. 333, 231-250 (1998)

Owing to a mistake, Fig. 2 was confused with an other figure. To rectify this unfortunate error, the correct Fig. 2 with ist caption is reprinted below.

[FIGURE] Fig. 2. Empirical [FORMULA]  versus V-I relation for dwarfs. Solid symbols are data from BLG94; crosses indicate AAM96 (for [FORMULA] [Fe/H] [FORMULA]); open circles with error bars indicate Code et al. (1976)

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© European Southern Observatory (ESO) 1998

Online publication: August 6, 1998