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- W98678416 abstract "The photospheric temperature of active stars is affected by the presence of cool starspots. The determination of the spot configuration and, in particular, spot temperatures and sizes, is important for understanding the role of the magnetic field in blocking the convective heating flux inside starspots. It has been demonstrated that a very sensitive diagnostic of surface temperature in late-type stars is the depth ratio of weak photospheric absorption lines (e.g. Gray & Johanson 1991, Catalano et al. 2002). We have shown that it is possible to reconstruct the distribution of the spots, along with their sizes and temperatures, from the application of a spot model to the light and temperature curves (Frasca et al. 2005). In this work, we present and briefly discuss results on spot sizes and temperatures for stars in various locations in the HR diagram." @default.
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- W98678416 date "2006-01-01" @default.
- W98678416 modified "2023-10-17" @default.
- W98678416 title "Starspot temperature along the HR diagram" @default.
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- W98678416 hasPublicationYear "2006" @default.
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