The chromospheric hypothesis for the T Tauri phenomenon

• 1 February 1984
• journal article
• Published by American Astronomical Society in The Astrophysical Journal
• Vol. 277, 725-737
• https://doi.org/10.1086/161744

Abstract

Keywords

• CHROMOSPHERE
• LATE STARS
• STELLAR EVOLUTION
• STELLAR MODELS
• T TAURI STARS
• ABSORPTION SPECTRA
• ABUNDANCE
• EMISSION SPECTRA
• LINE SPECTRA
• MAIN SEQUENCE STARS
• SPECTRAL ENERGY DISTRIBUTION
• STELLAR ATMOSPHERES
• STELLAR TEMPERATURE
• ULTRAVIOLET SPECTRA