An effective temperature calibration for solar type stars using equivalent width ratios. A fast and easy spectroscopic temperature estimation
Aims: Precise determination of the stellar effective temperature of solar type stars is extremely important for astrophysics. We present an effective temperature calibration for FGK dwarf stars using the line equivalent width ratios of spectral absorption lines. Methods: We used the automatic code ARES to measure the equivalent width for several
Sousa, S. G. et al.
Fecha de publicación:
3
2010