Figure 6 from Intrinsic Colors, Temperatures, and Bolometric Corrections of Pre-main-sequence Stars

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Intrinsic Colors, Temperatures, and Bolometric Corrections of Pre-main-sequence Stars

Authors: Mark J. Pecaut and Eric E. Mamajek

Pecaut & Mamajek 2013 The Astrophysical Journal Supplement Series 208 9.

Provider: AAS Journals

Caption: Figure 6.

SED for β Pic member V1005 Ori (K8IVe). Observed photometry (circles) with the best fit BT-Settl model photometry (crosses) from a T _eff = 3866 ± 18 K model (interpolated). Uncertainties are smaller than the symbol markers.

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