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.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
astro-ph.HE 2verdicts
UNVERDICTED 2representative citing papers
A combination of rotochemical heating with a large pairing gap and vortex creep explains the observed temperatures of PSR J0437-4715 and PSR B0950+08 while remaining consistent with upper limits on three other old pulsars.
citing papers explorer
-
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.
-
Neutron star heating vs. HST observations
A combination of rotochemical heating with a large pairing gap and vortex creep explains the observed temperatures of PSR J0437-4715 and PSR B0950+08 while remaining consistent with upper limits on three other old pulsars.