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The effective temperature scale of giant stars (F0–K5): II. Empirical calibration of $T_{{\rm eff}}$ versus colours and [Fe/H]

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Alonso, A., Arribas, S., Martínez-Roger, C.·1999·Astronomy and Astrophysics Supplement Series

Abstract

We present calibrations of the effective temperatures of giant stars versus [Fe/H] and colours , , , , , , , , , , and . These calibrations are based on a large sample of field and globular cluster stars which roughly cover spectral types from F0 to K5. Their effective temperatures, scaled to direct determinations via reliable angular diameter measurements, were derived by applying the infrared flux method. The empirical relations have been fitted to polynomials of the form by using the least squares method. The precision of the fits ranges from 40 K for to 170 K for . We tabulate intrinsic colours of giant stars in the ranges: 3500 K 8000 K; -3.0 . We also present the calibration of BC(V) as a function of log and metallicity. Finally, we compare the resulting scale of temperatures with previous works.

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Metadata

Authors
Alonso, A., Arribas, S., & Martínez-Roger, C.
Venue
Astronomy and Astrophysics Supplement Series
Publisher
EDP Sciences
Published
1999-12
Volume
140
Issue
3
Pages
261-277
ISSN
  • 0365-0138 (ISSN-L)
  • 1286-4846
OpenAlex
W1979257798
Cited by
1,019
References
0
FWCI
14.07
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: The effective temperature scale of giant stars (F0–K5): II. Empirical calibration of $T_{{\rm eff}}$ versus colours and [Fe/H]. https://app.cochat.ai/papers/10.1051/aas:1999521
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Alonso, A., Arribas, S., & Martínez-Roger, C. (1999). The effective temperature scale of giant stars (F0–K5): II. Empirical calibration of $T_{{\rm eff}}$ versus colours and [Fe/H]. Astronomy and Astrophysics Supplement Series. https://doi.org/10.1051/aas%3A1999521

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