Discovery of PSR J0125-5854, a 24 ms pulsar in a binary with orbital period ~834 days, low eccentricity, and likely helium white dwarf companion.
Fiore , author L
4 Pith papers cite this work, alongside 12 external citations. Polarity classification is still indexing.
4
Pith papers citing it
12
external citations · OpenAlex
fields
astro-ph.HE 4representative citing papers
Special relativistic simulations predict detectable radio emission from nightside magnetic structures around planets in pulsar winds, including for the known planet PSR J0636+5129 b.
Coherent timing solutions at 150 MHz for 17 pulsars from Irish LOFAR observations, including 7 without prior solutions.
Two FAST-discovered pulsars now have timing solutions, polarization profiles, and flux densities; one looks like an isolated partially recycled pulsar whose dispersion measure exceeds the maximum predicted by Galactic electron-density models.
citing papers explorer
-
Discovery of a 24-millisecond pulsar in a very long orbit with the Murchison Widefield Array
Discovery of PSR J0125-5854, a 24 ms pulsar in a binary with orbital period ~834 days, low eccentricity, and likely helium white dwarf companion.
-
Planets in Pulsar Winds
Special relativistic simulations predict detectable radio emission from nightside magnetic structures around planets in pulsar winds, including for the known planet PSR J0636+5129 b.
-
Pulsar timing solutions for 17 pulsars at 150 MHz from the Irish LOFAR station
Coherent timing solutions at 150 MHz for 17 pulsars from Irish LOFAR observations, including 7 without prior solutions.
-
Discovery and Timing Follow-Up of Two FAST-Discovered Pulsars from the FAST CRAFTS Survey
Two FAST-discovered pulsars now have timing solutions, polarization profiles, and flux densities; one looks like an isolated partially recycled pulsar whose dispersion measure exceeds the maximum predicted by Galactic electron-density models.