Results 41 to 50 of about 121,901 (271)
Fast radio bursts as giant pulses from young rapidly rotating pulsars [PDF]
We discuss possible association of fast radio bursts (FRBs) with supergiant pulses emitted by young pulsars (ages $\sim$ tens to hundreds of years) born with regular magnetic field but very short -- few milliseconds -- spin periods.
M. Lyutikov, L. Burzawa, S. Popov
semanticscholar +1 more source
Observations of the gamma-ray pulsar J1836+5925 at 111 MHz
We describe the 10-day radio observations of the gamma-ray pulsar J1836+5925. Observations were carried out in the Pushchino Radio Astronomical Observatory at the frequency of 111 MHz using the Large Phased Array of the Lebedev Physical Institute.
Timirkeeva Maria+3 more
doaj +1 more source
Multi-Messenger Astrophysics of a Millisecond Pulsar Orbiting around a Massive Black Hole
Extreme-mass-ratio and intermediate-mass-ratio binaries with a millisecond pulsar are gravitational-wave sources that emit also electromagnetic radiation.
Kinwah Wu
doaj +1 more source
Polarimetry of 600 pulsars from observations at 1.4 GHz with the Parkes radio telescope [PDF]
Over the past 13 years, the Parkes radio telescope has observed a large number of pulsars using digital filterbank backends with high time and frequency resolution and the capability for Stokes recording.
S. Johnston, M. Kerr
semanticscholar +1 more source
Pulsar wind nebulae created by fast-moving pulsars [PDF]
We review multiwavelength properties of pulsar wind nebulae created by supersonically moving pulsars and the effects of pulsar motion on the pulsar wind nebulae morphologies and the ambient medium.
O. Kargaltsev+3 more
semanticscholar +1 more source
Neste texto, descreve-se o conceito para o edifício Pulsar, uma estrutura arquitetónica reprogramável constituída por materiais texteis inteligentes com origem na nanotecnologia.
openaire +3 more sources
Gravitational waves from pulsars in the context of magnetic ellipticity
In one of our previous articles we have considered the role of a time dependent magnetic ellipticity on the pulsars’ braking indices and on the putative gravitational waves these objects can emit.
José C. N. de Araujo+2 more
doaj +1 more source
Post-main-sequence planetary system evolution [PDF]
The fates of planetary systems provide unassailable insights into their formation and represent rich cross-disciplinary dynamical laboratories. Mounting observations of post-main-sequence planetary systems necessitate a complementary level of theoretical
Dimitri Veras
doaj +1 more source
Dealing with the data imbalance problem on pulsar candidates sifting based on feature selection [PDF]
Pulsar detection has become an active research topic in radio astronomy recently. One of the essential procedures for pulsar detection is pulsar candidate sifting (PCS), a procedure of finding out the potential pulsar signals in a survey. However, pulsar candidates are always class-imbalanced, as most candidates are non-pulsars such as RFI and only a ...
arxiv +1 more source
Timing analysis for 20 millisecond pulsars in the Parkes Pulsar Timing Array [PDF]
We present timing models for 20 millisecond pulsars in the Parkes Pulsar Timing Array. The precision of the parameter measurements in these models has been improved over earlier results by using longer data sets and modelling the non-stationary noise. We
D. Reardon+24 more
semanticscholar +1 more source