[82.06] Matrix Lightcurve Inversion: HR 1099 Results and Comparison with other Methods

AAS Meeting #194 - Chicago, Illinois, May/June 1999
Session 82. A Stellar and Variable Star Melange
Display, Thursday, June 3, 1999, 9:20am-4:00pm, Southwest Exhibit Hall

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[82.06] Matrix Lightcurve Inversion: HR 1099 Results and Comparison with other Methods

L Crews (Vanderbilt U), R Harmon (Randolph Macon C), D S Hall (Vanderbilt U)

We have surface mapping results generated from wideband photometric data for several stars using Matrix Lightcurve Inversion (MLI). One of these stars, HR 1099=V711 Tauri, has been modeled and mapped using standard "trial-and-error" photometric methods and doppler imaging. The comparison of these various results is enlightening with respect to the capability of MLI as an improvement over older photometric methods and as a suitable replacement for doppler imaging when that technique is not viable.

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