Chemodynamical models of galactic evolution

2005 ◽  
pp. 159-173 ◽  
Author(s):  
A. Burkert ◽  
G. Hensler
Keyword(s):  
Galactic Evolution

The Galactic Evolution of Si, Ti, and O Isotopic Ratios

1999 ◽  
Vol 519 (1) ◽  
pp. 222-235 ◽  
Author(s):  
Conel M. O’D. Alexander ◽  
Larry R. Nittler
Keyword(s):  
Galactic Evolution ◽  
Isotopic Ratios

scholarly journals Galactic bulge giants: probing stellar and galactic evolution

2010 ◽  
Vol 517 ◽  
pp. A44 ◽  
Author(s):  
S. Uttenthaler ◽  
M. Stute ◽  
R. Sahai ◽  
J. A. D. L. Blommaert ◽  
M. Schultheis ◽  
...  
Keyword(s):  
Galactic Evolution ◽  
Galactic Bulge

Galactic evolution of 7Li: the interplay between novae and AGB stars

2001 ◽  
Vol 688 (1-2) ◽  
pp. 442-446
Author(s):  
C. Travaglio ◽  
D. Galli ◽  
S. Randich
Keyword(s):  
Galactic Evolution ◽  
Agb Stars

9Be abundances in dwarfs of intermediate metal deficiency: Impications for galactic evolution

1989 ◽  
Vol 157 (1-2) ◽  
pp. 41-46 ◽  
Author(s):  
J. E. Beckman ◽  
C. Abia ◽  
R. Rebolo
Keyword(s):  
Galactic Evolution ◽  
Metal Deficiency

High-precision abundances of elements in stars with asteroseismic ages

2017 ◽  
Vol 13 (S334) ◽  
pp. 166-169
Author(s):  
P. E. Nissen ◽  
V. Silva Aguirre ◽  
J. Christensen-Dalsgaard ◽  
R. Collet ◽  
F. Grundahl ◽  
...  
Keyword(s):  
High Precision ◽  
Main Sequence ◽  
Potential Problem ◽  
Galactic Evolution ◽  
The Other ◽  
Main Sequence Stars ◽  
Refractory Elements ◽  
Other Hand ◽  
New Information ◽  
Oscillation Frequencies

AbstractHigh-precision abundances of elements have been derived from HARPS-N spectra of F and G main-sequence stars having ages determined from oscillation frequencies delivered by the Kepler mission. The tight relations between abundance ratios of refractory elements, e.g., [Mg/Fe] and [Y/Mg], and stellar age previously found for solar twin stars are confirmed. These relations provide new information on nucleosynthesis and Galactic evolution. Abundance ratios between volatile and refractory elements, e.g., [C/Fe] and [O/Fe], show on the other hand a significant scatter at a given age, which may be related to planet-star interactions. This is a potential problem for chemical tagging studies.

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