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.
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2 Pith papers cite this work. Polarity classification is still indexing.
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2026 2representative citing papers
Direct N-body simulations independently confirm that preferential ejection of enriched RGB stars by an active black hole subsystem produces a transient overconcentration of pristine RGB stars in globular clusters that have lost substantial mass.
citing papers explorer
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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.
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Is the overconcentration of pristine populations in Galactic globular clusters real? An N-body approach to the problem
Direct N-body simulations independently confirm that preferential ejection of enriched RGB stars by an active black hole subsystem produces a transient overconcentration of pristine RGB stars in globular clusters that have lost substantial mass.