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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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Highly Cited
2013
Highly Cited
2013
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
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
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
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
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
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
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
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
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
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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