Results 241 to 250 of about 120,893 (256)
Magnetically Induced Rotating Rayleigh-Taylor Instability. [PDF]
J Vis Exp, 2017 Scase MM, Baldwin KA, Hill RJ.
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Cloning and characterization of a chitinase from Thermobifida fusca reveals Tfu_0580 as a thermostable and acidic endochitinase. [PDF]
Biotechnol Rep (Amst), 2018 Yan Q, Fong SS.
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Probing the gravitational Faraday rotation using quasar X-ray microlensing. [PDF]
Sci Rep, 2015 Chen B.
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Testing General Relativity with Pulsar Timing. [PDF]
Living Rev Relativ, 2003 Stairs IH.
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Physics of Neutron Star Crusts. [PDF]
Living Rev Relativ, 2008 Chamel N, Haensel P.
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Crab Pulsar Observations with AquEYE
AIP Conference Proceedings, 2009As is well known, the Crab pulsar displays a light curve with a characteristic double peak profile having a period of 33 milliseconds. Its pulse profile has been extensively monitored by several authors; it is also used for testing high‐speed photon counters. We have studied the optical light curve of the Crab pulsar by means of a novel photon counting
C. Germanà +10 more
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Frontiers of Physics, 2020
There are some similarities between bursts of repeating fast radio bursts (FRBs) and giant pulses (GPs) of pulsars. To explore possible relations between them, we study the cumulative energy distributions of these two phenomena using the observations of ...
Fen Lyu +8 more
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There are some similarities between bursts of repeating fast radio bursts (FRBs) and giant pulses (GPs) of pulsars. To explore possible relations between them, we study the cumulative energy distributions of these two phenomena using the observations of ...
Fen Lyu +8 more
semanticscholar +1 more source
Nature, 1969
WE have attempted optical observations of the Vela pulsar PSR 0833–45 (ref. 1) and measurement of linear and circular polarization in the Crab pulsar NP 0532 (refs. 2, 3, and unpublished work of R. Lynds, S. P. Maran and D. E. Trumbo) with a 74 inch telescope.
K. C. FREEMAN +3 more
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WE have attempted optical observations of the Vela pulsar PSR 0833–45 (ref. 1) and measurement of linear and circular polarization in the Crab pulsar NP 0532 (refs. 2, 3, and unpublished work of R. Lynds, S. P. Maran and D. E. Trumbo) with a 74 inch telescope.
K. C. FREEMAN +3 more
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Crab Pulsar Radiation Mechanism
Nature Physical Science, 1971SMITH has recently presented an oblique rotator model for the Crab pulsar1 in which the magnetic axis is inclined at an angle of 45° to the rotation axis and the observer's line of sight is at a latitude of about 20°. This model is in conflict with that discussed by Wampler et al.2, Kristian et al.3, Manchester4 and others, in which the magnetic axis ...
E. Tademaru, Richard N. Manchester
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Irregularities in the Crab Pulsar Wobble
Nature, 1970THIS article presents new measurements of the arrival times of optical pulses from the Crab pulsar, NP 0532. The observations were obtained at Hamburg Observatory (Bergedorf) with a 60 cm refractor and a data acquisition system with an on-line computer (PDP-8/S). Comparison of our results with those obtained by Boynton et al.1 and Richards et al.2 does
E. Høg, E. Lohsen
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