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Paper: Evidence for a Complex Distribution of Magnetic Field Strengths on the Flare Star AD Leo
Volume: 26, Cool Stars, Stellar Systems, and the Sun: Seventh Cambridge Workshop
Page: 252
Authors: Saar, S. H.
Abstract: I present a preliminary analysis of four Ti I lines from a high S/N IR spectrum of the flare star AD Leo. The lines show consistent evidence for a complex magnetic field distribution, and may be fit with either (a) fields arising from a single atmospheric component but having a large vertical gradient, or (b) a two component field with B_1 ~ 2 x B_2.
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