Stellar Streams Reveal the Mass Loss of Globular Clusters

Globular cluster (GC) streams, debris of stars tidally stripped from their progenitor GCs, have densities that correlate positively with the GC mass-loss rate. In this work, we employ a novel particle spray algorithm that can accurately reproduce the morphology of streams of various orbital types, e...

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Main Authors: Yingtian Chen, Hui Li, Oleg Y. Gnedin
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal Letters
Subjects:
Online Access:https://doi.org/10.3847/2041-8213/adaf93
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author Yingtian Chen
Hui Li
Oleg Y. Gnedin
author_facet Yingtian Chen
Hui Li
Oleg Y. Gnedin
author_sort Yingtian Chen
collection DOAJ
description Globular cluster (GC) streams, debris of stars tidally stripped from their progenitor GCs, have densities that correlate positively with the GC mass-loss rate. In this work, we employ a novel particle spray algorithm that can accurately reproduce the morphology of streams of various orbital types, enabling us to uncover the relationship between the GC mass-loss history and stream density profiles. Using recent discoveries of GC streams from Gaia Data Release 3, we present, for the first time, a catalog of directly observed mass-loss rates for 12 Galactic GCs, ranging from 0.5 to 200 M _⊙ Myr ^−1 . By fitting power-law relations between the mass-loss rate and key GC properties, we identify positive correlations with GC mass and orbital frequency, consistent with the predictions from N -body simulations.
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series The Astrophysical Journal Letters
spelling doaj-art-856b0ece97e640509de614db0202f2b62025-02-11T17:14:57ZengIOP PublishingThe Astrophysical Journal Letters2041-82052025-01-019802L1810.3847/2041-8213/adaf93Stellar Streams Reveal the Mass Loss of Globular ClustersYingtian Chen0https://orcid.org/0000-0002-5970-2563Hui Li1https://orcid.org/0000-0002-1253-2763Oleg Y. Gnedin2https://orcid.org/0000-0001-9852-9954Department of Astronomy, University of Michigan , Ann Arbor, MI 48109, USA ; ybchen@umich.eduDepartment of Astronomy, Tsinghua Univeristy , Beijing 100084, People’s Republic of China ; hliastro@tsinghua.edu.cnDepartment of Astronomy, University of Michigan , Ann Arbor, MI 48109, USA ; ybchen@umich.eduGlobular cluster (GC) streams, debris of stars tidally stripped from their progenitor GCs, have densities that correlate positively with the GC mass-loss rate. In this work, we employ a novel particle spray algorithm that can accurately reproduce the morphology of streams of various orbital types, enabling us to uncover the relationship between the GC mass-loss history and stream density profiles. Using recent discoveries of GC streams from Gaia Data Release 3, we present, for the first time, a catalog of directly observed mass-loss rates for 12 Galactic GCs, ranging from 0.5 to 200 M _⊙ Myr ^−1 . By fitting power-law relations between the mass-loss rate and key GC properties, we identify positive correlations with GC mass and orbital frequency, consistent with the predictions from N -body simulations.https://doi.org/10.3847/2041-8213/adaf93Stellar streamsGlobular star clustersStellar dynamicsGalaxy dynamics
spellingShingle Yingtian Chen
Hui Li
Oleg Y. Gnedin
Stellar Streams Reveal the Mass Loss of Globular Clusters
The Astrophysical Journal Letters
Stellar streams
Globular star clusters
Stellar dynamics
Galaxy dynamics
title Stellar Streams Reveal the Mass Loss of Globular Clusters
title_full Stellar Streams Reveal the Mass Loss of Globular Clusters
title_fullStr Stellar Streams Reveal the Mass Loss of Globular Clusters
title_full_unstemmed Stellar Streams Reveal the Mass Loss of Globular Clusters
title_short Stellar Streams Reveal the Mass Loss of Globular Clusters
title_sort stellar streams reveal the mass loss of globular clusters
topic Stellar streams
Globular star clusters
Stellar dynamics
Galaxy dynamics
url https://doi.org/10.3847/2041-8213/adaf93
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