The Anomalous Acceleration of PSR J2043+1711: Long-period Orbital Companion or Stellar Flyby?
Based on the rate of change of its orbital period, PSR J2043+1711 has a substantial peculiar acceleration of 3.5 ± 0.8 mm s ^–1 yr ^–1 , which deviates from the acceleration predicted by equilibrium Milky Way (MW) models at a 4 σ level. The magnitude of the peculiar acceleration is too large to be e...
Saved in:
Similar Items
-
Pulse Profile Variability of PSR J1022+1001 in NANOGrav Data
by: William Fiore, et al.
Published: (2025-01-01) -
Pulsar Cyclic Spectroscopy in the Partial-deconvolution Regime: Benefits and Limitations
by: Jacob E. Turner, et al.
Published: (2025-01-01) -
The NANOGrav 15 Yr Data Set: Removing Pulsars One by One from the Pulsar Timing Array
by: Gabriella Agazie, et al.
Published: (2025-01-01) -
The NANOGrav 15 yr Data Set: Harmonic Analysis of the Pulsar Angular Correlations
by: Gabriella Agazie, et al.
Published: (2025-01-01) -
The NANOGrav 12.5 yr Data Set: Probing Interstellar Turbulence and Precision Pulsar Timing with PSR J1903+0327
by: Abra Geiger, et al.
Published: (2025-01-01)