articleThe Astrophysical Journal Supplement SeriesSep 4, 2013BRONZE OA

INTRINSIC COLORS, TEMPERATURES, AND BOLOMETRIC CORRECTIONS OF PRE-MAIN-SEQUENCE STARS

MJMark J. PecautEEEric E. Mamajek
Indexed inarxivcrossrefdoaj

Abstract

We present an analysis of the intrinsic colors and temperatures of 5-30 Myr old pre-main sequence (pre-MS) stars using the F0 through M9 type members of nearby, negligibly reddened groups: Eta Cha cluster, TW Hydra Association, Beta Pic Moving Group, and Tucana-Horologium Association. To check the consistency of spectral types from the literature, we estimate new spectral types for 52 nearby pre-MS stars with spectral types F3 through M4 using optical spectra taken with the SMARTS 1.5-m telescope. Combining these new types with published spectral types, and photometry from the literature (Johnson-Cousins BVIc, 2MASS JHKs and WISE W1, W2, W3, and W4), we derive a new empirical spectral type-color sequence for…

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Authors

2
  • MJ
    Mark J. PecautCorresponding
  • EE
    Eric E. Mamajek

Topics & keywords

Keywords
  • Stars
  • Photometry (optics)
  • Stellar classification
  • T Tauri star
  • Main sequence
  • Effective temperature
  • Spectral line
  • Herbig Ae/Be star
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