Amanote Research
Register
Sign In
A Comparison Between the Relative Heavy Metal Abundance of the Extreme Halo Field Stars and Giant Stars of Globular Clusters
Symposium - International Astronomical Union
doi 10.1017/s0074180900145486
Full Text
Open PDF
Abstract
Available in
full text
Date
January 1, 1978
Authors
M. Spite
F. Spite
Publisher
Cambridge University Press (CUP)
Related search
Evidence of Helium Abundance Differences Between the Hyades Stars and Field Stars, and Between Hyades Stars and Coma Cluster Stars
Publications of the Astronomical Society of the Pacific
Astrophysics
Astronomy
Planetary Science
Space
Field Stars, Open Clusters, and the Galactic Abundance Gradient
Astronomical Journal
Astrophysics
Astronomy
Planetary Science
Space
Fast Rotating Massive Stars and the Origin of the Abundance Patterns in Galactic Globular Clusters
Astronomy and Astrophysics
Astrophysics
Astronomy
Planetary Science
Space
Convection in the Atmospheres and Envelopes of Turnoff and Giant Branch Stars of Globular Clusters
Astronomy and Astrophysics
Astrophysics
Astronomy
Planetary Science
Space
Variable Stars in the Metal-Rich Globular Clusters NGC 6388 and NGC 6441
International Astronomical Union Colloquium
On a Possible Relation Between Globular Clusters and Stars of High Velocity
Proceedings of the National Academy of Sciences of the United States of America
Multidisciplinary
A Photometric Survey for Variable Stars in Twelve Metal-Rich Globular Clusters
International Astronomical Union Colloquium
Chemical Composition of Halo Field Stars and the Chemical Evolution of the Halo
Highlights of Astronomy
Observations of Blue Straggler Stars in Globular Clusters
Proceedings of the International Astronomical Union
Astrophysics
Astronomy
Planetary Science
Space