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- W2085729175 abstract "High resolution, high S/N-ratio line profiles of the BY Draconis-type flare star EQ Vir obtained with the MMT are presently subjected to a novel Zeeman analysis procedure which includes radiative transfer effects and compensation for blends. A mean field of 2500 + or - 300 G covering 80 + or 15 percent of EQ Vir is determined. This constitutes the first positive detection of a magnetic field in a BY Draconis-type flare star, confirming that magnetic fields are present on these stars. The value of 2500 G obtained for the photospheric field strength is similar to the value derived by assuming equipartition of magnetic and thermal energy densities in the photosphere and scaling from the solar network fields, suggesting that equipartition may determine the mean field strength in the nonspotted portion of the flare star photosphere." @default.
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- W2085729175 date "1986-03-01" @default.
- W2085729175 modified "2023-09-27" @default.
- W2085729175 title "The magnetic field of the BY Draconis flare star EQ Virginis" @default.
- W2085729175 doi "https://doi.org/10.1086/164040" @default.
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