Fig. 6
Location of the stars observed in the Taurus Auriga region. The contours are low lying levels of CO integrated intensity from the Dame et al. (2001) survey. The red dots are stars in common between Ducourant et al. (2005) and Kenyon et al. (2008) master list of PMS stars in Taurus. The red crosses show the stars with precise distances (VLBA or VB+SB2) The blue crosses show the stars with masses measured by disk rotation.
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