SIMBAD references

2006A&A...450..735M - Astronomy and Astrophysics, volume 450, 735-746 (2006/5-1)

Effective temperature scale and bolometric corrections from 2MASS photometry.

MASANA E., JORDI C. and RIBAS I.

Abstract (from CDS):

We present a method to determine effective temperatures, angular semi-diameters and bolometric corrections for population I and II FGK type stars based on V and 2MASS IR photometry. Accurate calibration is accomplished by using a sample of solar analogues, whose average temperature is assumed to be equal to the solar effective temperature of 5777K. By taking into account all possible sources of error we estimate associated uncertainties to better than 1% in effective temperature and in the range 1.0-2.5% in angular semi-diameter for unreddened stars. Comparison of our new temperatures with other determinations extracted from the literature indicates, in general, remarkably good agreement. These results suggest that the effective temperaure scale of FGK stars is currently established with an accuracy better than 0.5%-1%. The application of the method to a sample of 10999 dwarfs in the Hipparcos catalogue allows us to define temperature and bolometric correction (K band) calibrations as a function of (V-K), [m/H] and logg. Bolometric corrections in the V and K bands as a function of Teff, [m/H] and logg are also given. We provide effective temperatures, angular semi-diameters, radii and bolometric corrections in the V and K bands for the 10999 FGK stars in our sample with the corresponding uncertainties.

Abstract Copyright:

Journal keyword(s): stars: fundamental parameters - stars: late-type - stars: sub-dwarfs - infrared: stars - techniques: photometric - methods: analytical

VizieR on-line data: <Available at CDS (J/A+A/450/735): table2.dat table3.dat>

Simbad objects: 10999

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2006A&A...450..735M and select 'bookmark this link' or equivalent in the popup menu


2021.05.11-22:12:05

© Université de Strasbourg/CNRS

    • Contact