The Astrophysical Journal Supplement Series· 2013Q1
INTRINSIC COLORS, TEMPERATURES, AND BOLOMETRIC CORRECTIONS OF PRE-MAIN-SEQUENCE STARS
- 2,324citations
- Q1SCImago
- 2013year
Short summary
A new empirical spectral type–color sequence for 5-30 Myr old pre-main-sequence (pre-MS) stars reveals deviations from dwarf star colors, with pre-MS stars being up to ~250 K cooler than their main-sequence counterparts for spectral types G5-K6.
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Astronomy and AstrophysicsPhysics and Astronomy