Probing Populations of Dark Stellar Remnants in the Globular Clusters 47 Tuc and Terzan 5 Using Pulsar Timing

We present a new method to combine multimass equilibrium dynamical models and pulsar timing data to constrain the mass distribution and remnant populations of Milky Way globular clusters (GCs). We first apply this method to 47 Tuc, a cluster for which there exists an abundance of stellar kinematic d...

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Váldodahkkit:	Peter J. Smith, Vincent Hénault-Brunet, Nolan Dickson, Mark Gieles, Holger Baumgardt
Materiálatiipa:	Artigo
Giella:	Inglês
Almmustuhtton:	IOP Publishing 2024-01-01
Ráidu:	The Astrophysical Journal
Fáttát:	Black holes Globular star clusters Millisecond pulsars Pulsars Star clusters Stellar dynamics
Liŋkkat:	https://doi.org/10.3847/1538-4357/ad77bc
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