SCEPtERbinary-package {SCEPtERbinary}R Documentation

A grid-based estimation tool for the age of stars in bynary systems

Description

The package estimates the age of stars in double-lined detached binary systems, given observational effective temperature, metallicity [Fe/H], mass, and radius of both stars. The results are obtained adopting a maximum likelihood technique on a grid of computed stellar models.

References

G. Valle, M. Dell'Omodarme, P.G. Prada Moroni, and S. Degl'Innocenti (2014). Uncertainties in grid-based estimates of stellar mass and radius. SCEPtER: Stellar CharactEristics Pisa Estimation gRid. A&A, 561, A125.

G. Valle, M. Dell'Omodarme, P.G. Prada Moroni, and S. Degl'Innocenti (2014). Uncertainties in asteroseismic grid-based estimates of stellar ages. SCEPtER: Stellar CharactEristics Pisa Estimation gRid. A&A, accepted.

G. Valle, M. Dell'Omodarme, P.G. Prada Moroni, and S. Degl'Innocenti (2014). Grid-based estimates of stellar ages in binary systems. SCEPtER: Stellar CharactEristics Pisa Estimation gRid. A&A, submitted.


[Package SCEPtERbinary version 0.1-1 Index]