Surface Maps of LO Pegasi May-July 2011 Generated via BVRI Light Curve Inversion

Details Surface Maps of LO Pegasi May-July 2011 Generated via BVRI Light Curve Inversion Surface Maps of LO Pegasi May-July 2011 Generated via BVRI Light Curve Inversion

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aas...21943311h&link_type=abstract

American Astronomical Society, AAS Meeting #219, #433.11

Astronomy and Astrophysics

Astronomy

Scientific paper

The young solar analog LO Pegasi is a rapidly rotating (P ≈ 10.2 hr) K8 main sequence star known to exhibit large cool spots on its surface. We present surface maps based on BVRI photometry obtained at Perkins Observatory from May-July 2011 and inverted with an algorithm which makes no a priori assumptions regarding the number of spots or their shapes, and compare the results to images generated from 2006-2010. This work was supported by the NSF REU Program.

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