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SIIA Público
SISTEMA INTEGRAL DE INFORMACIÓN ACADÉMICA - PÚBLICO
Título del libro: New Quests In Stellar Astrophysics Iii: A Panchromatic View Of Solar-Like Stars, With And Without Planets Título del capítulo: Empirical Calibration of the Physical Parameters of Solar-like Stars using uvby-Stromgren Photometry
SPECTRAL CLASSIFICATION; BETA PHOTOMETRY; NEIGHBORHOOD; CATALOG; COLOR
Resumen:
We present an empirical calibration of the physical parameters of A, F
and early G-type stars of luminosity class V. We have used a statistical
approach based on a sample of about 15 000 stars having both
uvby-Stromgren photomerty (Hauck & Mermilliod 1998) and spectral types
taken from SIMBAD. Stars closer than 70 pc have been considered
reddening-free. In this paper we present the results for 1900 stars
within 70 pc. Mean unreddened measurements have been used as input to
CHORIZOS (Malz-Apellaniz 2004). By assuming ``solar metallicity''
([Fe/H]=0), we have been able to determine effective temperatures
(T-eff) and surface gravities (log g) for each spectral type. We have
found a tight correlations among the observations and the derived
physical parameters; for example, T-eff can be expressed as a cubic
polynomial in (b - y)(0). From the distribution of colors and indices
for 128 stars and their associated physical parameters we have proposed
an alternative definition for solar-analogs: stars whose classification
is G2 V with (b - y)(0), = 0.3927 +/- 0.0190, (m(1))(0) = 0.1901 +/-
0.0143, and (c(1))(0) = 0.3302 +/- 0.0388, T-eff = 5930 +/- 145 K, and
log g = 4.70 +/- 0.33. These values are consistent with previous
empirical results; however, (m(1))(c), differs from a recent model-based
value for this index derived by Melendez et al. (2010). This discrepancy
points out the actual solar metallicity problem. We suggest that our
sample of solar analogs could be useful for searches of solar twins and
exoplanets.