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Decay of Planetary Debris Disks

  • Authors: G. H. Rieke, K. Y. L. Su, J. A. Stansberry, D. Trilling, G. Bryden, J. Muzerolle, B. White, N. Gorlova, E. T. Young, C. A. Beichman, K. R. Stapelfeldt, and D. C. Hines

Rieke et al. 2005 The Astrophysical Journal 620 1010.

  • Provider: AAS Journals

Caption: Fig. 2.

Slopes of debris disk SEDs. Data are from IRAS, 25 to 60 μm, or MIPS, 24 to 70 μm. Stars less than 25 Myr old are shown as dotted lines, between 25 and 200 Myr as dashed lines, and older than 200 Myr as solid lines.

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