Fig. 14 from Spitzer MIPS Observations of Stars in the β Pictoris Moving Group

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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. 14.

Plot of ﹩v\mathrm{sin}\,i﹩ (in km s⁻¹) vs. ﹩F_{\mathrm{meas}\,}/ F_{\mathrm{pred}\,}﹩ at 24 μm (top) and at 70 μm (bottom) for all of the BPMG G, K, and M stars considered here. While certainly not conclusive, these figures are reminiscent of effects seen in younger clusters such as Orion.

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