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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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