Globular cluster luminosity function as distance indicator
M. Rejkuba (ESO, Germany)

TL;DR
The paper reviews the use of the Globular Cluster Luminosity Function as a distance indicator, highlighting its historical significance, recent insights, and the complexities affecting its accuracy due to galaxy and cluster evolution.
Contribution
It provides a comprehensive overview of recent observational and theoretical studies showing the dependencies and limitations of the GCLF as a distance indicator.
Findings
GCLF peak magnitude is influenced by galaxy type and environment.
Recent data suggest systematic dependencies affecting distance estimates.
Complex physics of cluster formation impacts GCLF reliability.
Abstract
Globular clusters are among the first objects used to establish the distance scale of the Universe. In the 1970-ies it has been recognized that the differential magnitude distribution of old globular clusters is very similar in different galaxies presenting a peak at M_V ~ -7.5. This peak magnitude of the so-called Globular Cluster Luminosity Function has been then established as a secondary distance indicator. The intrinsic accuracy of the method has been estimated to be of the order of ~0.2 mag, competitive with other distance determination methods. Lately the study of the Globular Cluster Systems has been used more as a tool for galaxy formation and evolution, and less so for distance determinations. Nevertheless, the collection of homogeneous and large datasets with the ACS on board HST presented new insights on the usefulness of the Globular Cluster Luminosity Function as distance…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
