output
19962026
most citedA bright millisecond radio burst of extragalactic origin

2k citations

Showing 2006 · astro-phShow all

7 papers · 2 filters

astro-ph2006★ 13 cited

Correlation between X-ray Lightcurve Shape and Radio Arrival Time in the Vela Pulsar

A. Lommen, J. Donovan, C. Gwinn +6

We report the results of simultaneous observations of the Vela pulsar in X-rays and radio from the RXTE satellite and the Mount Pleasant Radio Observatory in Tasmania. We sought co…

astro-ph2006★ 70 cited

A Survey of 56 Mid-latitude EGRET Error Boxes for Radio Pulsars

F. Crawford, M. S. E. Roberts, J. W. T. Hessels +4

We have conducted a radio pulsar survey of 56 unidentified gamma-ray sources from the 3rd EGRET catalog which are at intermediate Galactic latitudes (5 deg. < |b| < 73 deg.). For e…

astro-ph2006★ 565 cited

The Parkes multibeam pulsar survey: VI. Discovery and timing of 142 pulsars and a Galactic population analysis

D. R. Lorimer, A. J. Faulkner, A. G. Lyne +11

[ABRIDGED] We present the discovery and follow-up observations of 142 pulsars found in the Parkes 20-cm multibeam pulsar survey of the Galactic plane. These new discoveries bring t…

astro-ph2006★ 1 cited

Galactic Abundance Patterns via Peimbert Types I & II Planetary Nebulae

J. B. Milingo, K. B. Kwitter, R. B. C. Henry +1

Planetary Nebulae (PNe) abundance patterns have long been used to note signatures of nuclear processing and to trace the distribution of metals throughout galaxies. We present abun…

astro-ph2006★ 2 cited

The Sulfur Abundance Anomaly in Planetary Nebulae

R. B. C. Henry, J. N. Skinner, K. B. Kwitter +1

The failure of S and O abundances in most planetary nebulae to display the same strong direct correlation that is observed in extragalactic H II regions represents one of the most…

astro-ph2006★ 50 cited

The Parallax and Proper Motion of PSR J0030+0451

Andrea N. Lommen, Richard A. Kipphorn, David J. Nice +3

We report the parallax and proper motion of millisecond pulsar J0030+0451, one of thirteen known isolated millisecond pulsars in the disk of the Galaxy. We obtained more than 6 yea…