Abstract
The rate of production of heavy elements is rediscussed using the models of Arnett (1978) for late stage nucleosynthesis in massive stars, the M(M,) relationship of Chiosi et al. (1978b) for losing mass models in the core H and He-Burning phases, and the stellar birth rate of Miller and Scalo (1978). Contrary to that found by Wheeler et al (1978), we do not encounter the difficulty of heavy element overproduction. The explosive nucleosynthesis from massive stars is still compatible with the observed abundance distribution of the solar system, and a stellar birth rate decreasing over the history of the galactic disk.
Chiosi, C
[1]
- Padua Univ. (Italy). Istituto di Astronomia
Citation Formats
Chiosi, C.
Effect of mass loss by stellar wind on the chemical enrichment of the galaxy.
Germany: N. p.,
1979.
Web.
Chiosi, C.
Effect of mass loss by stellar wind on the chemical enrichment of the galaxy.
Germany.
Chiosi, C.
1979.
"Effect of mass loss by stellar wind on the chemical enrichment of the galaxy."
Germany.
@misc{etde_5022233,
title = {Effect of mass loss by stellar wind on the chemical enrichment of the galaxy}
author = {Chiosi, C}
abstractNote = {The rate of production of heavy elements is rediscussed using the models of Arnett (1978) for late stage nucleosynthesis in massive stars, the M(M,) relationship of Chiosi et al. (1978b) for losing mass models in the core H and He-Burning phases, and the stellar birth rate of Miller and Scalo (1978). Contrary to that found by Wheeler et al (1978), we do not encounter the difficulty of heavy element overproduction. The explosive nucleosynthesis from massive stars is still compatible with the observed abundance distribution of the solar system, and a stellar birth rate decreasing over the history of the galactic disk.}
journal = []
volume = {80:2}
journal type = {AC}
place = {Germany}
year = {1979}
month = {Jan}
}
title = {Effect of mass loss by stellar wind on the chemical enrichment of the galaxy}
author = {Chiosi, C}
abstractNote = {The rate of production of heavy elements is rediscussed using the models of Arnett (1978) for late stage nucleosynthesis in massive stars, the M(M,) relationship of Chiosi et al. (1978b) for losing mass models in the core H and He-Burning phases, and the stellar birth rate of Miller and Scalo (1978). Contrary to that found by Wheeler et al (1978), we do not encounter the difficulty of heavy element overproduction. The explosive nucleosynthesis from massive stars is still compatible with the observed abundance distribution of the solar system, and a stellar birth rate decreasing over the history of the galactic disk.}
journal = []
volume = {80:2}
journal type = {AC}
place = {Germany}
year = {1979}
month = {Jan}
}