The Chemical Properties of Milky Way and M31 Globular Clusters. II. Stellar Population Model Predictions

Astronomical Journal - United States
doi 10.1086/427715
Full Text
Abstract

Available in full text

Date
Authors
Publisher

IOP Publishing

Related search

Are Some Milky Way Globular Clusters Hosted by Undiscovered Galaxies?

Astrophysical Journal Letters
AstrophysicsAstronomyPlanetary ScienceSpace
2016English

Stellar Astrophysics: The Mystery of Globular Clusters

Nature
Multidisciplinary
2016English

Chemical Abundances of Seven Outer Halo M31 Globular Clusters From the Pan-Andromeda Archaeological Survey

Proceedings of the International Astronomical Union
AstrophysicsAstronomyPlanetary ScienceSpace
2016English

Spectroscopic Explorations of Milky Way Stellar Populations

English

Formation of Globular Clusters and the First Stellar Generations

Symposium - International Astronomical Union
1988English

Multicolor Photometry and Age Estimates of Globular Clusters in M31

Highlights of Astronomy
2005English

Insights Into the Chemical Composition of the Metal-Poor Milky Way Halo Globular Cluster NGC 6426

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2017English

Studying Milky Way Structure Using Stellar Populations

Proceedings of the International Astronomical Union
AstrophysicsAstronomyPlanetary ScienceSpace
2006English

A Stellar Relic From the Early Milky Way

Nature
Multidisciplinary
2002English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2024 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy