Results 91 to 100 of about 116,704 (219)
Calculation of radar signals delay to second order in the frame of the General Relativity Theory
From the Schwarzschild metric, the light delay due to a gravitational field is calculated to second order approximation in the gravitational potential. We analize the contribution of the second order terms for strong gravitational fields as the generated
Joaquín Valerio Grefa, Carlos A. Marín
doaj +1 more source
X-ray observations of the Large Magellanic Cloud pulsar PSR B0540-69 and its PWN
PSR B0540-69 is a young pulsar in the Large Magellanic Cloud that has similar properties with respect to the Crab Pulsar, and is embedded in a Pulsar Wind Nebula.
A. De Rosa +48 more
core +1 more source
Early phases of different types of isolated neutron star
Two Galactic isolated strong X-ray pulsars seem to be in the densest environments compared to other types of Galactic pulsar. X-ray pulsar J1846-0258 can be in an early phase of anomalous X-ray pulsars and soft gamma repeaters if its average braking ...
AŞKIN ANKAY +12 more
core +1 more source
Adaptive Filters Revisited - RFI Mitigation in pulsar observations
Pulsar detection and timing experiments are applications where adaptive filters seem eminently suitable tools for radio-frequency-interference (RFI) mitigation.
B. Dawson +11 more
core +1 more source
Detection of radio emission from the gamma-ray pulsar J1732-3131 at 327 MHz
Although originally discovered as a radio-quiet gamma-ray pulsar, J1732-3131 has exhibited intriguing detections at decameter wavelengths. We report an extensive follow-up of the pulsar at 327 MHz with the Ooty radio telescope.
Joshi, Bhal Chandra +6 more
core +1 more source
Spin Tilts in the Double Pulsar Reveal Supernova Spin Angular-Momentum Production
The system PSR J0737-3039 is the only binary pulsar known to consist of two radio pulsars (PSR J0737-3039 A and PSR J0737-3039 B). This unique configuration allows measurements of spin orientation for both pulsars: pulsar A's spin is tilted from the ...
Dessart +17 more
core +1 more source
PSR J0437-4715 is a millisecond pulsar (MSP) thought to be ``pair formation starved'' (having limited pair cascades due to magnetic photon absorption).
de Jager, O. C., Tiplady, A., Venter, C.
core +2 more sources
E. ASSÉO, D. BEAUFILS, R. PELLAT
openaire +1 more source
We report the discovery of a young and energetic pulsar in the Parkes multibeam survey of the Galactic plane. PSR J1016-5857 has a rotation period of 107 ms and period derivative of 8e-14, implying a characteristic age of 21 kyr and spin-down luminosity ...
A. G. Lyne +14 more
core +1 more source
Search for a Correlation Between Radio Giant Pulses and VHE Photons of the Crab Pulsar
The Crab pulsar is a unique source of pulsar radio emission. Its regular pulse structure is visible over the entire electromagnetic spectrum from radio to GeV ranges.
N. Lewandowska +2 more
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