Effective temperature of A and F stars from Balmer line profiles, and the Infrared Flux Method. I. Two AM stars: the Sun and Procyon as standards.

Astronomy and Astrophysics – Astrophysics

Scientific paper


  [ 0.00 ] – not rated yet Voters 0   Comments 0

Please leave your Comment & Rating

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.