Results 211 to 220 of about 16,963 (231)
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]
Astrophys J, 2016 Barnard M, Venter C, Harding AK.
europepmc +1 more source
Some of the next articles are maybe not open access.
Related searches:
Related searches:
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 +2 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 +2 more sources
1992
A study of the flux density and component emission of four millisecond radio pulsars shows that on average millisecond radio pulsars have steeper spectra than slow period pulsars. The results of flux density measurements of four millisecond pulsars, PSRs 1620-26, 1821-24, 1855+09, and 1937+21, have been made to determine their spectral indices in the ...
R. S. Foster, D. C. Backer, L. Fairhead
openaire +1 more source
A study of the flux density and component emission of four millisecond radio pulsars shows that on average millisecond radio pulsars have steeper spectra than slow period pulsars. The results of flux density measurements of four millisecond pulsars, PSRs 1620-26, 1821-24, 1855+09, and 1937+21, have been made to determine their spectral indices in the ...
R. S. Foster, D. C. Backer, L. Fairhead
openaire +1 more source
Il Nuovo Cimento C, 1990
In this paper we briefly review the observed parameters of the presently known millisecond pulsars and the general ideas about their formation secenario. We describe the results of recent searche and unbiased surveys, and we discuss some possible observation strategies.
openaire +1 more source
In this paper we briefly review the observed parameters of the presently known millisecond pulsars and the general ideas about their formation secenario. We describe the results of recent searche and unbiased surveys, and we discuss some possible observation strategies.
openaire +1 more source
Nature, 1987
The recent discovery1,2 of a 3-millisecond pulsar in the globular cluster M28 (NGC6626) suggests that a few per cent of type I super novae (of which there are several subcategories, all associated with old stellar populations) form neutron stars. If the contact-binary white dwarf model for type Is is invoked3, it seems probable that millisecond pulsars
openaire +1 more source
The recent discovery1,2 of a 3-millisecond pulsar in the globular cluster M28 (NGC6626) suggests that a few per cent of type I super novae (of which there are several subcategories, all associated with old stellar populations) form neutron stars. If the contact-binary white dwarf model for type Is is invoked3, it seems probable that millisecond pulsars
openaire +1 more source
Millisecond pulsar radiation properties
Journal of Astrophysics and Astronomy, 1995Two investigations of millisecond pulsar radiation are discussed: average total intensity pulse morphology and individual pulse to pulse fluctuations. The average emission profiles of millisecond pulsars are compared with those of slower pulsars in the context of polar cap models.
openaire +1 more source
Binary and Millisecond Pulsars
2014The first evidence for neutron stars residing in binaries came in the early 60s when Giacconi et al. (1962) discovered the first extrasolar X-ray source, Sco X\(-\)1.
openaire +1 more source