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19952023
most citedA Massive Pulsar in a Compact Relativistic Binary

3.9k citations · 36.1k across the 290 of their papers we have counts for

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Showing 2000 · astro-phShow all

6 papers · 2 filters

astro-ph2000★ 67 cited

A radio supernova remnant associated with the young pulsar J1119-6127

Fronefield Crawford, B. M. Gaensler, V. M. Kaspi +4

We report on Australia Telescope Compact Array observations in the direction of the young high magnetic-field pulsar J1119-6127. In the resulting images we identify a non-thermal r…

astro-ph2000★ 54 cited

PSR J1740-3052 - a pulsar with a massive companion

I. H. Stairs, R. N. Manchester, A. G. Lyne +14

We report on the discovery of a binary pulsar, PSR J1740-3052, during the Parkes multibeam survey. Timing observations of the 570-ms pulsar at Jodrell Bank and Parkes show that it…

astro-ph2000★ 63 cited

Long-Term RXTE Monitoring of the Anomalous X-ray Pulsar 1E 1048.1-5937

Victoria M. Kaspi, Fotis P. Gavriil, Deepto Chakrabarty +2

We report on long-term monitoring of the anomalous X-ray pulsar (AXP) 1E 1048.1-5937 using the Rossi X-ray Timing Explorer (RXTE). The timing behavior of this pulsar is different f…

astro-ph2000★ 81 cited

A Glitch in an Anomalous X-ray Pulsar

V. M. Kaspi, J. R. Lackey, D. Chakrabarty

We report the detection of a sudden spin-up of the 11 s anomalous X-ray pulsar 1RXS J170849.0-4000910 in regular timing observations made with the Rossi X-ray Timing Explorer. The…

astro-ph2000★ 256 cited

Discovery of Two High-Magnetic-Field Radio Pulsars

F. Camilo, V. M. Kaspi, A. G. Lyne +6

We report the discovery of two young isolated radio pulsars with very high inferred magnetic fields. PSR J1119-6127 has period P = 0.407 s, and the largest period derivative known…

astro-ph2000★ 18 cited

A Search for Sub-millisecond Pulsations in Unidentified FIRST and NVSS Radio Sources

Fronefield Crawford, Victoria M. Kaspi, Jon F. Bell

We have searched 92 unidentified sources from the FIRST and NVSS 1400 MHz radio survey catalogs for radio pulsations at 610 MHz. The selected radio sources are bright, have no iden…