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

open access: yesSci Rep, 2018
Murakami M, Arefiev A, Zosa MA.
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Navigation using binary pulsars

Science China Physics, Mechanics and Astronomy, 2012
The issue of navigation using binary pulsars is investigated in this paper. We show how the effect of the binary motion is incorporated in the navigation measurement equation. Necessary reference systems and time scales are introduced and the transformation between different time scales is derived. Based mainly on Damour and Deruelle’s binary model and
Liangwei Huang   +3 more
semanticscholar   +3 more sources

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   +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

Binary pulsars in magnetic field versus spin period diagram

, 2013
We analyzed 186 binary pulsars (BPSRs) in the magnetic field versus spin period (B-P) diagram, where their relations to the millisecond pulsars (MSPs) can be clearly shown.
Y. Y. Pan, Na Wang, Chunlin Zhang
semanticscholar   +2 more sources

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