Published March 15, 1982
| Version v1
Journal article
CNO isotopes and galactic chemical evolution
Description
In order to quantitatively reproduce the chemical abundance gradient and the age-metallicity relation observed in the disk of the Galaxy, numerical models of galactic chemical evolution have been computed under different assumptions on the star formation and infall rates. The best fit to the observed data is obtained for a model with a constant star formation rate and a uniform infall rate of 5 x 10-3 M/sub sun/ kpc-2 yr-1. Models with other star formation laws do not reproduce the observed data as well
Additional details
Publishing Information
- Journal Title
- Astrophys. J.
- Journal Volume
- 254
- Journal Issue
- 2
- Series
- Astrophys. J.
- Journal Page Range
- 699-707
- ISSN
- 0004-637X
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 14722313
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- CARBON ISOTOPES; CHEMICAL COMPOSITION; COSMOCHEMISTRY; GALACTIC EVOLUTION; GALAXIES; ISOTOPE RATIO; NITROGEN ISOTOPES; NUCLEOSYNTHESIS; NUMERICAL SOLUTION; OXYGEN ISOTOPES
- Descriptors DEC
- CHEMISTRY