Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1978
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978mmsai..49..781g&link_type=abstract
(Consiglio Nazionale delle Ricerche, Convegno sulle Metodologie di Trattamento dell'Informazione, Trieste, Nov. 24, 25, 1977 and
Astronomy and Astrophysics
Astronomy
Flare Stars, Magnetic Stars, Stellar Evolution, Stellar Magnetic Fields, T Tauri Stars, Variable Stars, Magnetohydrodynamic Stability, Main Sequence Stars, Photosphere, Statistical Correlation, Ultraviolet Radiation
Scientific paper
Probable manifestations of magnetism in UV Ceti flare stars and T Tauri stars are considered. A hydromagnetic model of variability is proposed for interpreting the main features of T Tauri stars. It is concluded that: (1) T Tauri stars of spectral types F through M have strong large-scale magnetic fields and are the predecessors of main-sequence stars of spectral types A through G; (2) T Tauri activity is a manifestation of instability in magnetic inhibition of stellar brightness; and (3) UV Ceti-type flare activity is a manifestation of instability in local magnetic fields on generally stable stars and is energized, directly or indirectly, by magnetic fields.
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