scispace - formally typeset
Journal ArticleDOI

The Chemical Composition of Red Giants. III. Further CNO Isotopic and s-Process Abundances in Thermally Pulsing Asymptotic Giant Branch Stars

Verne V. Smith, +1 more
- 01 Feb 1990 - 
- Vol. 72, pp 387
Reads0
Chats0
About
This article is published in Astrophysical Journal Supplement Series.The article was published on 1990-02-01. It has received 339 citations till now. The article focuses on the topics: Asymptotic giant branch & Barium star.

read more

Citations
More filters
Journal ArticleDOI

The Apache Point Observatory Galactic Evolution Experiment (APOGEE)

Steven R. Majewski, +96 more
TL;DR: In this article, the Hungarian National Research, Development and Innovation Office (K-119517) and Hungarian National Science Foundation (KNFI) have proposed a method to detect the presence of asteroids in Earth's magnetic field.
Journal ArticleDOI

Nucleosynthesis in asymptotic giant branch stars: Relevance for galactic enrichment and solar system formation

TL;DR: In this paper, a review of nucleosynthesis in AGB stars outlining the development of theoretical models and their relationship to observations is presented, focusing on the new high-resolution codes with high accuracy.
Journal ArticleDOI

Evolution of Asymptotic Giant Branch Stars

TL;DR: The current status of modeling the evolution and nucleosynthesis of asymptotic giant branch (AGB) stars is reviewed in this paper, where several constraints and methods are available to improve the models.
Journal ArticleDOI

Neutron Capture in Low Mass Asymptotic Giant Branch Stars: Cross Sections and Abundance Signatures

TL;DR: Recently improved information on the stellar (n, γ) cross sections of neutron magic nuclei at N = 82, and in particular of 142Nd, turn out to represent a sensitive test for models of s-process nucleosynthesis as mentioned in this paper.
Journal ArticleDOI

Evolution and nucleosynthesis in low-mass asymptotic giant branch stars. II.Neutron capture and the s-process

TL;DR: In this article, a new analysis of neutron capture occurring in low-mass asymptotic giant branch (AGB) stars suffering recurrent thermal pulses is presented, where the authors use dedicated evolutionary models for stars of initial mass in the range 1 to 3 M? and metallicity from solar to half solar.
Related Papers (5)