Image Details
Caption: Figure 13.
Cumulative distribution functions of stellar mass ( M *), fractional infrared luminosity ( L IR/ L *), and grain temperature ( T gr) for debris disks around old ( t age ⩾ 300 Myr) and young ( t age < 300 Myr) stars. The colors have the same meaning as in Figure 12.
© 2014. The American Astronomical Society. All rights reserved.