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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. 8.

Star+disk models of the 10 stars considered for more sophisticated modeling; see text for discussion as to how they were selected and the details of the modeling. Notation is as in Figs. 14: the ﹩x﹩‐axis plots the log of the wavelength in microns, and the ﹩y﹩‐axis plots ﹩\mathrm{log}\,( \lambda F_{\lambda }) ﹩ in cgs units (ergs s−1 cm−2). Points gleaned from the literature are diamonds, boxes are detections or upper limits from IRAS, and circles are new MIPS points. Downward‐pointing arrows indicate upper limits.

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