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Star Formation History in the Solar Vicinity

  • Authors: G. Bertelli and E. Nasi

Bertelli & Nasi 2001 The Astronomical Journal 121 1013.

  • Provider: AAS Journals

Caption: Fig. 3.

(a) Values of ﹩\chi ^{2}_{\mathrm{MS}\,}﹩ computed for the SFR const‐const model and with IMF x = 2.35 to test the simulated sample (produced with constant SFR and x = 2.35). Tb varies between Ti and Tf, spaced by 1 Gyr. Each line corresponds to a different value of Ib. Squares indicate models whose probability P from the K‐S test is greater than 0.1. (b) Same as (a) but for ﹩\chi ^{2}_{\mathrm{red}\,}﹩. Solid triangles indicate that condition Rb is satisfied; open triangles correspond to models that satisfy condition Rc.

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