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Spitzer MIPS Observations of Stars in the β Pictoris Moving Group

  • Authors: L. M. Rebull, K. R. Stapelfeldt, M. W. Werner, V. G. Mannings, C. Chen, J. R. Stauffer, P. S. Smith, I. Song, D. Hines, and F. J. Low

Rebull et al. 2008 The Astrophysical Journal 681 1484.

  • Provider: AAS Journals

Caption: Fig. 12.

Ratio of measured to predicted 70 μm flux as a function of time for objects in the literature, as described in the text; gray times symbols or upper limits correspond to our objects from the BPMG and Tuc‐Hor. The horizontal dotted line corresponds to the ﹩F_{\mathrm{meas}\,}/ F_{\mathrm{pred}\,}=2﹩ cutoff between disks and photospheres discussed in § 3.2.

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