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A VLBI experiment using a remote atomic clock via a coherent fibre link. [PDF]
Clivati C+15 more
europepmc +1 more source
The effect of an offset polar cap dipolar magnetic field on the modeling of the Vela pulsar's <i>γ</i>-ray light curves. [PDF]
Barnard M, Venter C, Harding AK.
europepmc +1 more source
Relativistic Binaries in Globular Clusters. [PDF]
Benacquista MJ.
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Testing General Relativity with Pulsar Timing. [PDF]
Stairs IH.
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The influence of the enhanced vector meson sector on the properties of the matter of neutron stars. [PDF]
Bednarek I, Manka R, Pienkos M.
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CONSTRAINING RELATIVISTIC BOW SHOCK PROPERTIES IN ROTATION-POWERED MILLISECOND PULSAR BINARIES. [PDF]
Wadiasingh Z+4 more
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Searching for Millisecond Pulsars in Globular Clusters at Parkes: Further Results
Andrea Possenti+5 more
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Nature, 1982
The radio properties of 4C21.53 have been an enigma for many years. First, the object displays interplanetary scintillations (IPS) at 81 MHz, indicating structure smaller than 1 are s, despite its low galactic latitude (−0.3°)1. IPS modulation is rare at low latitudes because of interstellar angular broadening. Second, the source has an extremely steep
Backer, D. C.+4 more
openaire +3 more sources
The radio properties of 4C21.53 have been an enigma for many years. First, the object displays interplanetary scintillations (IPS) at 81 MHz, indicating structure smaller than 1 are s, despite its low galactic latitude (−0.3°)1. IPS modulation is rare at low latitudes because of interstellar angular broadening. Second, the source has an extremely steep
Backer, D. C.+4 more
openaire +3 more sources