Image Details
Caption: Figure 9.
Comparison between the spectrum of V380 Ori B (black) and those of six M4-M9 dwarf field standard stars (red; Kirkpatrick et al. 1991; data from Burgasser et al. 2004, 2008) with different extinctions, showing good correspondence for M5–M6 stars with low extinction. The regions most affected by telluric absorption are shaded in gray, and were not used in the fits.
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