Results 31 to 40 of about 777,035 (267)
Axion resonances in binary pulsar systems [PDF]
We investigate the extent to which resonances between an oscillating background of ultra-light axion and a binary Keplerian system can affect the motion of the latter.
Mor Rozner+4 more
semanticscholar +1 more source
Interpretation of Binary Pulsar Observations [PDF]
The nature, dynamics and evolution of the three known radio pulsar binaries are discussed. The system containing 1913+16 appears to comprise two ~1.4 M⊙ components, and to undergo orbital decay as predicted by general relativity. It is proposed that 1913+16 has a neutron star companion and that 0655+64 and 0820+02 have white dwarf companions which ...
Blandford, R. D., DeCampli, W. M.
openaire +5 more sources
Radiation Dosimetry of Binary Pulsars [PDF]
Companion stars exposed to high energy radiation from a primary neutron star or accreting black hole can experience significant spallation of their heavy elements, so that their atmospheres would be extremely rich in lithium, beryllium, and especially boron. In this paper we note that the detection or non-detection of these elements, and their relative
Biman B. Nath, David Eichler
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Constraints on Undetected Long-period Binaries in the Known Pulsar Population
Although neutron star–black hole binaries have been identified through mergers detected in gravitational waves, a pulsar–black hole binary has yet to be detected.
Megan L. Jones+3 more
doaj +1 more source
Optical Identification of the Shortest-period Spider Pulsar System M71E
M71E is a spider pulsar (i.e., a millisecond pulsar with a tight binary companion) with the shortest known orbital period of P = 53.3 minutes, which was discovered by Pan et al.
Zhuokai Liu, Subo Dong
doaj +1 more source
A pulsar in a binary with a compact object in the mass gap between neutron stars and black holes [PDF]
Some compact objects observed in gravitational wave events have masses in the gap between known neutron stars (NSs) and black holes (BHs). The nature of these mass gap objects is unknown, as is the formation of their host binary systems. We report pulsar
E. Barr+24 more
semanticscholar +1 more source
Binary and Millisecond Pulsars [PDF]
77 pages, 30 figures, available on-line at http://www.livingreviews.org/lrr-2005 ...
openaire +13 more sources
Discovery and Timing of Millisecond Pulsars in the Globular Cluster M5 with FAST and Arecibo
We report on a comprehensive multiwavelength study of the pulsars in the globular cluster (GC) M5, including the discovery of M5G, a new compact noneclipsing “black widow” pulsar.
Lei Zhang+31 more
doaj +1 more source
The High Time Resolution Universe Pulsar Survey - XIII. PSR J1757-1854, the most accelerated binary pulsar [PDF]
We report the discovery of PSR J1757$-$1854, a 21.5-ms pulsar in a highly-eccentric, 4.4-h orbit around a neutron star (NS) companion. PSR J1757$-$1854 exhibits some of the most extreme relativistic parameters of any known pulsar, including the strongest
A. Cameron+34 more
semanticscholar +1 more source
Decade long RXTE monitoring observations of Be/X-ray binary pulsar EXO 2030+375 [PDF]
We present a comprehensive timing and spectral studies of Be/X-ray binary pulsar EXO 2030+375 using extensive Rossi X-ray Timing Explorer observations from 1995 till 2011, covering numerous Type I and 2006 Type II outbursts.
Prahlad R. Epili+3 more
semanticscholar +1 more source