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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. 5.

Plot of ﹩K_{s}﹩ vs. ﹩K_{s}-[ 24] ﹩ for all of the objects considered here. Plus signs are objects from the BPMG; circles are objects from Tuc‐Hor. The objects with excesses at 24 μm, selected by a combination of techniques, are indicated by name; see text for discussion as to how the objects with excesses were selected.

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