Image Details
Caption: Fig. 6.
Evolution of metal mass density buildup inferred from the SFH, assuming (a) SalA IMF and (b) BG IMF. The gray shaded and hatched regions come from the 1 and 3 σ confidence regions around the SFH ﹩T=4﹩ MeV fits respectively. The triangles at ﹩z=0﹩ are from Calura & Matteucci (2004), and the open circles at ﹩z=0﹩ and ≈2.5 are from Dunne et al. (2003).
© 2006. The American Astronomical Society. All rights reserved. Printed in U.S.A.