Site Map
Contacts
Follow us on Facebook Follow us on Twitter YouTube channel
Centro de Astrofísica da Universidade do Porto

uvby-β photometry of solar twins
The solar colors, model atmospheres, and the Teff and metallicity scales

J. Meléndez, W. J. Schuster, J. S. Silva, I. Ramírez, L. Casagrande, P. Coelho

Abstract
Aims. Solar colors have been determined on the uvby–β photometric system to test absolute solar fluxes, to examine colors predicted by model atmospheres as a function of stellar parameters (Teff, log g, [Fe/H]), and to probe zero-points of Teff and metallicity scales.
Methods. New uvby–β photometry is presented for 73 solar-twin candidates. Most stars of our sample have also been observed spectroscopically to obtain accurate stellar parameters. Using the stars that most closely resemble the Sun, and complementing our data with photometry available in the literature, the solar colors on the uvby–β system have been inferred. Our solar colors are compared with synthetic solar colors computed from absolute solar spectra and from the latest Kurucz (ATLAS9) and MARCS model atmospheres. The zero-points of different Teff and metallicity scales are verified and corrections are proposed.
Results. Our solar colors are (b - y) = 0.4105±0.0015, m1, = 0.2122±0.0018, c1, = 0.3319±0.0054, and β = 2.5915±0.0024. The (b-y) and m1, colors obtained from absolute spectrophotometry of the Sun agree within 3-σ with the solar colors derived here when the photometric zero-points are determined from either the STISHST observations of Vega or an ATLAS9 Vegamodel, but the c1, and β synthetic colors inferred from absolute solar spectra agree with our solar colors only when the zero-points based on the ATLAS9 model are adopted. The Kurucz solar model provides a better fit to our observations than the MARCS model. For photometric values computed from the Kurucz models, (b - y) and m1, are in excellent agreement with our solar colors independently of the adopted zero-points, but for c1, and β agreement is found only when adopting the ATLAS9 zero-points. The c1, color computed from both the Kurucz and MARCS models is the most discrepant, probably revealing problems either with the models or observations in the u band. The Teff calibration of Alonso and collaborators has the poorest performance (~140 K off), while the relation of Casagrande and collaborators is the most accurate (within 10 K).We confirm that the Ramírez & Meléndez uvby metallicity calibration, recommended by Árnadóttir and collaborators to obtain [Fe/H] in F, G, and K dwarfs, needs a small (~10%) zero-point correction to place the stars and the Sun on the same metallicity scale. Finally, we confirm that the c1 index in solar analogs has a strong metallicity sensitivity.

Keywords
stars: atmospheres - stars: fundamental parameters - stars: solar-type - Sun: fundamental parameters

Notes
Based on observations collected at the H.L. Johnson 1.5m telescope at the Observatorio Astronómico Nacional at San Pedro Mártir, Baja California, México.
Tables 1-3 and 5 are only available in electronic form at http://www.aanda.org

Astronomy and Astrophysics
Volume 522, Page A98_1
November 2010

>> PDF>> ADS>> DOI

Institute of Astrophysics and Space Sciences

Institute of Astrophysics and Space Sciences (IA) is a new but long anticipated research infrastructure with a national dimension. It embodies a bold but feasible vision for the development of Astronomy, Astrophysics and Space Sciences in Portugal, taking full advantage and fully realizing the potential created by the national membership of the European Space Agency (ESA) and the European Southern Observatory (ESO). IA resulted from the merging the two most prominent research units in the field in Portugal: the Centre for Astrophysics of the University of Porto (CAUP) and the Center for Astronomy and Astrophysics of the University of Lisbon (CAAUL). It currently hosts more than two-thirds of all active researchers working in Space Sciences in Portugal, and is responsible for an even greater fraction of the national productivity in international ISI journals in the area of Space Sciences. This is the scientific area with the highest relative impact factor (1.65 times above the international average) and the field with the highest average number of citations per article for Portugal.

Proceed on CAUP's website|Go to IA website