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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3 Pith papers cite this work. Polarity classification is still indexing.
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2026 3verdicts
UNVERDICTED 3representative citing papers
Diffractive interstellar scintillation can produce the observed spectral features in CU Vir's coherent radio emission at 400 MHz for a small emitting region of 0.01 solar radii.
Survey continuation yields FRB20110220A, RRAT J0404+53, new data on J2028+28, and evidence that single-pulse detection rates vary with Galactic coordinates, implying a faint Galactic population.
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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The effect of interstellar scattering on coherent radio emission from stars: the case of CU Vir
Diffractive interstellar scintillation can produce the observed spectral features in CU Vir's coherent radio emission at 400 MHz for a small emitting region of 0.01 solar radii.
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The Northern High Time Resolution Universe pulsar survey: III. Single-pulse search continuation, follow-up observations, and initial results
Survey continuation yields FRB20110220A, RRAT J0404+53, new data on J2028+28, and evidence that single-pulse detection rates vary with Galactic coordinates, implying a faint Galactic population.