Results 31 to 40 of about 31,557 (257)
Advances in Space Research, 1998 14 pages, Latex, aas2pp4.sty, To appear in Satellite and Ground Based Studies of Radio Pulsars, proceedings of the 31st Scientific Assembly of ...
openaire +2 more sources
Estimating the Evolution of Sparks in the Partially Screened Gap of Pulsars from Subpulse Drifting
The Astrophysical Journal, 2023 A novel scheme has been developed to show that the observed phase behavior associated with subpulse drifting from two pulsars, J1034−3224 and J1720−2933, can be used to obtain the magnetic field configuration in the partially screened gap (PSG).
Rahul Basu +2 more
doaj +1 more source
The origin of single radio pulsars
, 1999 By comparing relative rates of supernovae versus formation rates of single radio pulsars, recycled pulsars, binary pulsars and X-ray binaries we put strong limits on the progenitors of radio pulsars and on the requirement of an asymmetry in the supernova.
Heuvel, Edward van den +1 more
core +2 more sources
30 Glitches in slow pulsars [PDF]
, 2006 We have analyzed 5.5 years of timing observations of 7 'slowly' rotating radio pulsars, made with the Westerbork Synthesis Radio Telescope. We present improved timing solutions and 30, mostly small, new glitches.
Arzoumanian +35 more
core +3 more sources
Mode Changing in PSR B0844-35 and PSR B1758-29 with Enhanced Emission at the Profile Centers
The Astrophysical Journal, 2023 We have studied the single pulse emission from two pulsars, PSR B0844-35 and PSR B1758-29, over a wide frequency range of 300–750 MHz using the upgraded Giant Metrewave Radio Telescope.
Rahul Basu +2 more
doaj +1 more source
The Zoo of Isolated Neutron Stars
Universe, 2023 In this brief review, I summarize our basic knowledge about different types of isolated neutron stars. I discuss radio pulsars, central compact objects in supernova remnants, magnetars, nearby cooling neutron stars (also known as the magnificent seven ...
Sergei B. Popov
doaj +1 more source
The KaVA and KVN Pulsar Project
, 2014 We present our work towards using the Korean VLBI (Very Long Baseline Interferometer) Network (KVN) and VLBI Exploration of Radio Astronomy (VERA) arrays combined into the KVN and VERA Array (KaVA) for observations of radio pulsars at high frequencies ($\
Dodson, Richard +6 more
core +1 more source
Modeling the non-recycled Fermi gamma-ray pulsar population [PDF]
, 2013 We use Fermi Gamma-ray Space Telescope detections and upper limits on non-recycled pulsars obtained from the Large Area Telescope (LAT) to constrain how the gamma-ray luminosity L depends on the period P and the period derivative \dot{P}.
Burnett, T. H. +5 more
core +3 more sources
Radio pulsar variability [PDF]
Proceedings of the International Astronomical Union, 2012 AbstractPulsars are potentially the most remarkable physical laboratories we will ever use. Although in many senses they are extremely clean systems there are a large number of instabilities and variabilities seen in the emission and rotation of pulsars.
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, 2004 PhD Thesis, Utrecht University 2004, with a summary in Dutch. 108 pages, 55 low-resolution figures.
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