Variability of M giant stars based on em Kepler photometry: general characteristics
Solar and Stellar Astrophysics
2014-05-08 v1
Abstract
Small amounts of pre-solar grains have survived in the matrices of primitive meteorites and interplanetary dust particles. Their detailed study in the laboratory with modern analytical tools provides highly accurate and detailed information with regard to stellar nucleosynthesis and evolution, grain formation in stellar atmospheres, and Galactic Chemical Evolution. Their survival puts constraints on conditions they were exposed to in the interstellar medium and in the Early Solar System.
Keywords
Cite
@article{arxiv.1405.1624,
title = {Variability of M giant stars based on em Kepler photometry: general characteristics},
author = {E. Bányai and L. L. Kiss and members of KASC WG12},
journal= {arXiv preprint arXiv:1405.1624},
year = {2014}
}
Comments
3 pages, 1 figures, conference proceeding