Bayesian Hierarchical Modelling of Initial-Final Mass Relations Across Star Clusters
Bayesian Hierarchical Modelling of Initial-Final Mass Relations Across Star Clusters
About this item
Full title
Author / Creator
Publisher
Ithaca: Cornell University Library, arXiv.org
Journal title
Language
English
Formats
Publication information
Publisher
Ithaca: Cornell University Library, arXiv.org
Subjects
More information
Scope and Contents
Contents
The initial-final mass relation (IFMR) of white dwarfs (WDs) plays an important role in stellar evolution. To derive precise estimates of IFMRs and explore how they may vary among star clusters, we propose a Bayesian hierarchical model that pools photo- metric data from multiple star clusters. After performing a simulation study to show the benefit...
Alternative Titles
Full title
Bayesian Hierarchical Modelling of Initial-Final Mass Relations Across Star Clusters
Authors, Artists and Contributors
Identifiers
Primary Identifiers
Record Identifier
TN_cdi_proquest_journals_2073813018
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2073813018
Other Identifiers
E-ISSN
2331-8422
DOI
10.48550/arxiv.1806.06733
