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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. 2.

(a) Shape of the SFR, as described in § 3.2 for the const‐const model, where Tb is the time of the rate change and Ib is the ratio of the SFR at the final time, Tf, to its value at Tb. (b) Same as (a), but for the var‐var model. In both panels the final time, Tf, is the same for all the shapes, but it is plotted separately for clarity.

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