Results 191 to 200 of about 2,637 (230)

Gravitational wave content and stability of uniformly, rotating, triaxial neutron stars in general relativity. [PDF]

Phys Rev D, 2017
Tsokaros A, Ruiz M, Paschalidis V, Shapiro SL, Baiotti L, Uryū K.   +5 more
europepmc   +1 more source

Novel X-ray Communication Based XNAV Augmentation Method Using X-ray Detectors. [PDF]

Sensors (Basel), 2015
Song S, Xu L, Zhang H, Bai Y.
europepmc   +1 more source

The Relativistic Binary Pulsar B1913+16

, 2002
J. M. Weisberg, J. H. Taylor
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Insights into conscious cognitive information processing. [PDF]

Front Behav Neurosci
Dere E.
europepmc   +1 more source

Separating astrophysical sources from indirect dark matter signals. [PDF]

Proc Natl Acad Sci U S A, 2015
Siegal-Gaskins JM.
europepmc   +1 more source

Generation of ultrahigh field by micro-bubble implosion. [PDF]

Sci Rep, 2018
Murakami M, Arefiev A, Zosa MA.
europepmc   +1 more source

One-Dimensional Relativistic Self-Gravitating Systems. [PDF]

Entropy (Basel)
Mann RB.
europepmc   +1 more source

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A Millisecond Pulsar in an Eclipsing Binary

Nature, 1988
We report the discovery of a remarkable pulsar with period 1.6 ms, moving in a nearly circular 9.17 hour orbit around a low mass companion star. At an observing frequency of 430 MHz, the pulsar, PSR 1957+20, is eclipsed once each orbit for about 50 minutes.
A. S. Fruchter, James Taylor, D. R. Stinebring   +2 more
openaire   +2 more sources

Binary X-Ray Pulsars

Nature, 1977
As X-ray astronomy enters the Einstein era when faint, distant, and exotic X-ray sources are being investigated, we thought it might be useful to review some of the progress made over the past decade on a class of relatively nearby objects that have contributed richly to our understanding of astrophysics — the binary X-ray pulsars.
Paul C. Joss, Saul Rappaport
openaire   +3 more sources