Periodic Q-mode modulation in PSR J18250935 (PSR B182209)
arXiv:1903.01989 · doi:10.1093/mnras/stz650
Abstract
PSR J18250935 (PSR B182209) switches between radio-quiet (Q-mode) and radio-bright (B-mode) modes. The Q-mode is known to have a periodic fluctuation that modulates both the interpulse and the main pulse with the same period. Earlier investigators argued that the periodic Q-mode modulation is associated with drifting subpulses. We report on single-pulse observations of PSR J18250935 that were made using the Parkes 64-m radio telescope with a central frequency of 1369 MHz. The high-sensitivity observations revealed that the periodic Q-mode modulation is in fact a periodic longitude-stationary intensity modulation occurring in the interpulse and the main pulse. The fluctuation spectral analysis showed that the modulation period is about , where is the rotation period of the pulsar. Furthermore, we confirm that the modulation patterns in the interpulse and the main pulse are phase-locked. Specifically, the intensities of the interpulse and the immediately following main pulse are more highly correlated than for the main pulse and interpulse at any other lag. Polarization properties of the strong and weak Q-mode states are different, even for the trailing part of the main pulse which does not show the periodic intensity modulation.
7 pages, 8 figures, 1 table; accepted for publication in MNRAS
References in corpus (12)
- The ATNF Pulsar Catalogue
- PSRCHIVE and PSRFITS An Open Approach to Radio Pulsar Data Storage and Analysis
- Switched magnetospheric regulation of pulsar spin-down
- A periodically active pulsar giving insight into magnetospheric physics
- Pulsar Nulling and Mode Changing
- Polarimetry of 600 pulsars from observations at 1.4 GHz with the Parkes radio telescope
- Meterwavelength Single-pulse Polarimetric Emission Survey II: The phenomenon of Drifting Subpulses
- Deep Analyses of Nulling in Arecibo Pulsars Reveal Further Periodic Behavior
- Meterwavelength Single-pulse Polarimetric Emission Survey III: The Phenomenon of Nulling in Pulsars
- On the pulse--width statistics in radio pulsars. I. Importance of the interpulse emission
- The main- interpulse interaction of PSR B1702-19
- Simultaneous X-ray and radio observations of the radio-mode switching pulsar PSR B1822-09
Cited by in corpus (13)
- Periodic Modulation : Newly emergent emission behaviour in Pulsars
- Periodic mode changing in PSR J1048-5832
- Explaining high-braking indice of magnetars SGR 0501+4516 and 1E 2259+586 using the double magnetic-dipole model
- Rapid Modification of Neutron Star Surface Magnetic Field: A proposed mechanism for explaining Radio Emission State Changes in Pulsars
- A polarization census of bright pulsars using the Ultra-Wideband Receiver on the Parkes radio telescope
- Radio emission features in different modes of PSR J0826+2637 (B0823+26)
- The dissipation of toroidal magnetic fields and spin-down evolution of young and strongly magnetized pulsars
- Nulling and subpulse drifting in PSR J1727-2739
- Periodic and Phase-locked Modulation in PSR B1929+10 Observed with FAST
- Emission Variation of a Long-period Pulsar Discovered by the Five-hundred-meter Aperture Spherical Radio Telescope (FAST)
- Science Using Single-Pulse Exploration with Combined Telescopes. I. The mode switching, flaring, and single-pulse morphology of PSR B1822-09
- Unveiling the emission properties of three long-period pulsars using FAST
- Main and interpulse interaction in PSRs J1842+0358 and J1926+0737: evidence for interpole communication