Results 311 to 313 of about 82,088 (313)

Chemical evolution in the Milky Way Disk

AIP Conference Proceedings, 2006
Classical models of galactic evolution predict a smooth rise in heavy‐element abundance (metallicity) with time. We test this prediction with a new, large and unbiased sample of long‐lived stars in the solar neighbourhood and find that several of the key tests fail to support the classical predictions.
openaire   +3 more sources

Chemo-Spectral Evolution of the Milky way and of Spiral Disks

Astrophysics and Space Science, 1999
Our model and its application to the Milky Way are discussed in detail in Boissier & Prantzos (1998). The stellar yields of Woosley & Weaver (1995) are used to compute the chemical evolution, while the spectral one is coherently followed with the stellar evolution tracks of the Geneva group (Schaller et al. (1992), Charbonnel et al.
Samuel Boissier, Nikos Prantzos
openaire   +2 more sources

The Disk of the Milky Way

Annals of the New York Academy of Sciences, 1992
openaire   +2 more sources