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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. 1.

SEDs for all the BPMG targets discussed in § 1. 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. The stellar model that is plotted is selected from the Kurucz‐Lejeune grid (see text for discussion), normalized to the ﹩K_{s}﹩ band as observed; the simple disk model shown here is described in the text. The dotted line is the disk component alone, and the dashed line is the sum of the disk‐plus‐star model when more than one data point describes the disk.

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