Metal Abundances of Damped Lyα Systems and the Chemical Evolution of Spiral Galaxies
1995 ◽
Vol 164
◽
pp. 457-457
Keyword(s):
Our chemical evolution models describe in detail the enrichment process of a number of individual elements from 12C to 56Fe, including delayed SNI contributions. Variation of the characteristic timescale of star formation (SF) t∗ not only results in differences in the abundance evolution but also changes abundance ratios of elements originating from different nucleosvnthetic sites, as e.g. [C/O], [O/Fe], or [Mg/Fe].
1995 ◽
Vol 164
◽
pp. 424-424
Keyword(s):
2006 ◽
Vol 2
(S235)
◽
pp. 313-313
1999 ◽
Vol 171
◽
pp. 196-203
Keyword(s):
2018 ◽
Vol 14
(A30)
◽
pp. 265-265
Keyword(s):
2009 ◽
Vol 5
(S265)
◽
pp. 247-248
Keyword(s):
Keyword(s):
2006 ◽
Vol 2
(S235)
◽
pp. 376-380
◽
Keyword(s):
2020 ◽
Vol 495
(4)
◽
pp. 4548-4556