Exploring the Chemical Evolution of Globular Clusters and their Stars : Observational Constraints on Atomic Diffusion and Cluster Pollution in NGC 6752 and M4
Through the cosmic matter cycle, the chemical evolution of the Milky Way is imprinted in the elemental abundance patterns of late-type stars (spectral types F to K). Due to their long lifetimes ( 1 Hubble time), these stars are of particular importance when it comes to studying the build-up of eleme...
Main Author: | Gruyters, Pieter |
---|---|
Format: | Doctoral Thesis |
Language: | English |
Published: |
Uppsala universitet, Observationell astrofysik
2014
|
Subjects: | |
Online Access: | http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-230182 http://nbn-resolving.de/urn:isbn:978-91-554-9008-9 |
Similar Items
-
Exploring the Chemical Composition and Double Horizontal Branch of the Bulge Globular Cluster NGC 6569
by: Johnson, Christian I., et al.
Published: (2018) -
Chemical Complexity in the Eu-enhanced Monometallic Globular NGC 5986
by: Johnson, Christian I., et al.
Published: (2017) -
The in situ origin of the globular cluster NGC 6388 from abundances of Sc, V, and Zn of a large sample of stars
by: Bragaglia, A., et al.
Published: (2022) -
A study of stellar population of intermediate-age globular cluster NGC 2249
by: Zhongmu Li, et al.
Published: (2020-06-01) -
Long Period Variable Stars in the Globular Cluster M5 (NGC 5904)
by: Pellegrin, Kyle S.
Published: (2020)