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Periodontal evaluation:Class:Pt:Gingiva:Ord:PSR scale

Known as: Periodontal evaluation:Class:Point in time:Gingiva:Ordinal:PSR scale, PSR SCALE:clase:punto en el tiempo:encía:ordinal:PSR SCALE, Periodontal evaluation Gingiva PSR scale 
 
National Institutes of Health

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EvaluationGingiva

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Highly Cited
2013
Highly Cited
2013
Synchronous X-ray and Radio Mode Switches: A Rapid Global Transformation of the Pulsar Magnetosphere
Pondering Pulsars Pulsars are rapidly rotating, magnetized neutron stars that are powered by the loss of rotational energy… Expand
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Highly Cited
2013
Highly Cited
2013
The Spin-down of PSR J0821-4300 and PSR J1210-5226: Confirmation of Central Compact Objects as Anti-Magnetars
Using XMM-Newton and Chandra, we measure period derivatives for the second and third known pulsars in the class of central… Expand
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Highly Cited
2011
Highly Cited
2011
A study of 315 glitches in the rotation of 102 pulsars
The rotation of more than 700 pulsars has been monitored using the 76-m Lovell Telescope at Jodrell Bank. Here we report on a new… Expand
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Highly Cited
2010
Highly Cited
2010
X-ray variability and evidence for pulsations from the unique radio pulsar/X-ray binary transition object FIRST J102347.6+003841
We report on observations of the unusual neutron-star binary system FIRST J102347.6+003841 carried out using the XMM-Newton… Expand
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Highly Cited
2009
Highly Cited
2009
Radio Detection of LAT PSRs J1741-2054 and J2032+4127: No Longer Just Gamma-ray Pulsars
Sixteen pulsars have been discovered so far in blind searches of photons collected with the Large Area Telescope on the Fermi… Expand
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Highly Cited
2008
Highly Cited
2008
Avalanche dynamics of radio pulsar glitches
We test statistically the hypothesis that radio pulsar glitches result from an avalanche process, in which angular momentum is… Expand
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Highly Cited
2007
Highly Cited
2007
Pulse Profiles, Spectra, and Polarization Characteristics of Nonthermal Emissions from the Crab-like Pulsars
We discuss nonthermal emission mechanisms of the Crab-like pulsars with both a two-dimensional electrodynamic study and a three… Expand
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Highly Cited
2002
Highly Cited
2002
TIMING OF MILLISECOND PULSARS IN NGC 6752: EVIDENCE FOR A HIGH MASS-TO-LIGHT RATIO IN THE CLUSTER CORE
Using pulse timing observations, we have obtained precise parameters, including positions with ~20 mas accuracy, of five… Expand
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Highly Cited
2000
Highly Cited
2000
A 700 Year-old Pulsar in the Supernova Remnant Kesteven 75
Since their discovery 30 years ago, pulsars have been understood to be neutron stars born rotating rapidly (~10-100 ms). These… Expand
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Highly Cited
1999
Highly Cited
1999
SNR G320.4–01.2 and PSR B1509–58: new radio observations of a complex interacting system
We describe radio continuum and spectral-line observations of the source G320.4–01.2 (MSH 15–52) and the coincident young pulsar… Expand
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