Stellar streams encode the initial mass function of globular clusters, recovered as a declining power-law with slope 1.3 for streams above 1000 solar masses.
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Bayesian latent model augments negative-binomial globular cluster scaling with a Gaussian observation layer for error propagation and releases Nimble/PyMC code.
Globular cluster deficits in several Coma galaxies, revealed by Voronoi density maps and asymmetry tests, provide evidence for environmental stripping.
citing papers explorer
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Inferring Globular Cluster Initial Mass Function from Stellar Streams
Stellar streams encode the initial mass function of globular clusters, recovered as a declining power-law with slope 1.3 for streams above 1000 solar masses.
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Modeling Globular Cluster Counts with Bayesian Latent Models
Bayesian latent model augments negative-binomial globular cluster scaling with a Gaussian observation layer for error propagation and releases Nimble/PyMC code.
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Evidence for Environmental Stripping in the Coma Cluster
Globular cluster deficits in several Coma galaxies, revealed by Voronoi density maps and asymmetry tests, provide evidence for environmental stripping.