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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 2.

Comparison of B −  V, VI C , J −  H, HK S , K S W1, and K S W2 vs. VK S of young stars from β Pic, η Cha, TWA, and Tuc-Hor moving groups (circles) with the dwarf color locus described in Appendix C and the giant color locus from Bessell & Brett (1988), except the B −  V giant locus, which is from Alonso et al. (1999). Spectral types corresponding to the VK S colors of dwarfs are plotted along the top. Objects with a known near-IR or IR excess have been excluded (see Table 1).

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