A comparison between X-shooter spectra and PHOENIX models across the HR-diagram
Aims: The path towards robust near-infrared extensions of stellar population models involves the confrontation between empirical and synthetic stellar spectral libraries across the wavelength ranges of photospheric emission. Indeed, the theory of stellar emission enters all population synthesis models, even when this is only implicit in the
Lançon, A. et al.
Fecha de publicación:
5
2021