JWST observations of Terzan 5 reveal multiple stellar populations with ages of 12.5 and 4.7 Gyr, plus hints of a 3.8 Gyr component, suggesting a multi-epoch formation history.
Title resolution pending
4 Pith papers cite this work. Polarity classification is still indexing.
4
Pith papers citing it
years
2026 4representative citing papers
A Gibbs sampling technique marginalizes over photon-to-Gaussian assignments to fit timing and noise models to discrete gamma-ray arrival times while accounting for pulse-profile uncertainty.
A phase-coherent 20-year timing solution for PSR J1905+0154A yields precise spin, orbital and astrometric parameters, identifies a helium white dwarf companion of 0.17-0.19 solar masses, and indicates the system may be unbound from NGC 6749.
Fifteen new millisecond pulsars discovered in 47 Tucanae with MeerKAT, raising the cluster total to 42 and including a black widow system and an eccentric binary with a massive companion.
citing papers explorer
-
The multi-age stellar populations of Terzan 5 as revealed by JWST
JWST observations of Terzan 5 reveal multiple stellar populations with ages of 12.5 and 4.7 Gyr, plus hints of a 3.8 Gyr component, suggesting a multi-epoch formation history.
-
Timing Gamma-ray Pulsars using Gibbs Sampling
A Gibbs sampling technique marginalizes over photon-to-Gaussian assignments to fit timing and noise models to discrete gamma-ray arrival times while accounting for pulse-profile uncertainty.
-
The one and the only: the pulsar - white dwarf system in NGC 6749
A phase-coherent 20-year timing solution for PSR J1905+0154A yields precise spin, orbital and astrometric parameters, identifies a helium white dwarf companion of 0.17-0.19 solar masses, and indicates the system may be unbound from NGC 6749.
-
Fifteen new millisecond pulsars in 47 Tucanae
Fifteen new millisecond pulsars discovered in 47 Tucanae with MeerKAT, raising the cluster total to 42 and including a black widow system and an eccentric binary with a massive companion.