We discuss four recycled pulsars found in Arecibo drift-scan searches. PSR J1944+0907 has a spin period of 5.2 ms and is isolated. The 5.8-ms pulsar J1453+19 may have a low-mass companion. We discuss these pulsars in the context of isolated millisecond pulsar formation and the minimum spin period of neutron stars. The isolated 56-ms pulsar J0609+2130 is possibly the remnant of a disrupted double neutron star binary. The 41-ms pulsar J1829+2456 is in a relativistic orbit. Its companion is most likely another neutron star, making this the eighth known double neutron star binary system
We report the discovery of the millisecond pulsar (MSP) PSR J1950+2414 (P=4.3 ms) in a binary system...
Millisecond pulsars are thought to be neutron stars that have been spun-up by accretion of matter fr...
In this paper, we present the results of timing observations of PSRs J1949+3106 and J1950+2414, two ...
We report on timing and single-pulse observations of 17 pulsars discovered at the Arecibo observator...
We report on eight millisecond pulsars (MSPs) in binary systems discovered with the Arecibo L-Band F...
We report on eight millisecond pulsars (MSPs) in binary systems discovered with the Arecibo L-Band F...
We report on eight millisecond pulsars (MSPs) in binary systems discovered with the Arecibo L-Band F...
We report the discovery of the millisecond pulsar (MSP) PSR J1950+2414 (P = 4.3 ms) in a binary syst...
Millisecond pulsars are thought to be neutron stars that have been spun-up by accretion of matter fr...
We report the discovery of PSR J1906+0746, a young 144 ms pulsar in a highly relativistic 3.98 hr or...
We report the discovery and initial follow-up of a double neutron star (DNS) system, PSR J1946+2052,...
We present the discovery and phase-coherent timing of four highly dispersed millisecond pulsars (MSP...
We report the discovery and initial follow-up of a double neutron star (DNS) system, PSR J1946+2052,...
We present the discovery and phase-coherent timing of four highly dispersed millisecond pulsars (MSP...
Millisecond pulsars are thought to be neutron stars that have been spun-up by accretion of matter fr...
We report the discovery of the millisecond pulsar (MSP) PSR J1950+2414 (P=4.3 ms) in a binary system...
Millisecond pulsars are thought to be neutron stars that have been spun-up by accretion of matter fr...
In this paper, we present the results of timing observations of PSRs J1949+3106 and J1950+2414, two ...
We report on timing and single-pulse observations of 17 pulsars discovered at the Arecibo observator...
We report on eight millisecond pulsars (MSPs) in binary systems discovered with the Arecibo L-Band F...
We report on eight millisecond pulsars (MSPs) in binary systems discovered with the Arecibo L-Band F...
We report on eight millisecond pulsars (MSPs) in binary systems discovered with the Arecibo L-Band F...
We report the discovery of the millisecond pulsar (MSP) PSR J1950+2414 (P = 4.3 ms) in a binary syst...
Millisecond pulsars are thought to be neutron stars that have been spun-up by accretion of matter fr...
We report the discovery of PSR J1906+0746, a young 144 ms pulsar in a highly relativistic 3.98 hr or...
We report the discovery and initial follow-up of a double neutron star (DNS) system, PSR J1946+2052,...
We present the discovery and phase-coherent timing of four highly dispersed millisecond pulsars (MSP...
We report the discovery and initial follow-up of a double neutron star (DNS) system, PSR J1946+2052,...
We present the discovery and phase-coherent timing of four highly dispersed millisecond pulsars (MSP...
Millisecond pulsars are thought to be neutron stars that have been spun-up by accretion of matter fr...
We report the discovery of the millisecond pulsar (MSP) PSR J1950+2414 (P=4.3 ms) in a binary system...
Millisecond pulsars are thought to be neutron stars that have been spun-up by accretion of matter fr...
In this paper, we present the results of timing observations of PSRs J1949+3106 and J1950+2414, two ...