Results 31 to 40 of about 28,625 (211)
Optical Identification of the Shortest-period Spider Pulsar System M71E
The Astrophysical Journal, 2023 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
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Binary and Other Recycled Pulsars [PDF]
Symposium - International Astronomical Union, 1992 Binary pulsars and others with weak fields and rapid rotation now number several dozen and appear to have been spun up by close binary mass transfer. Some are lineal descendents of X-ray binaries; others may result from accretion-induced collapse of binary white dwarfs or from captures, exchanges, and collisions in clusters. Seven accurate neutron star
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Looking for Light Pseudoscalar Bosons in the Binary Pulsar System J0737-3039 [PDF]
, 2005 We present numerical calculations of the photon-light-pseudoscalar-boson conversion in the recently discovered binary pulsar system J0737-3039. Light pseudoscalar bosons (LPBs) oscillate into photons in the presence of strong magnetic fields.
Arnaud Dupays +4 more
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Symposium - International Astronomical Union, 1981 There are now three radio frequency pulsars known to be in binary systems: PSRs 1913+16, 0820+02, and 0655+64. The first of these, discovered in 1974, moves in a tight, highly eccentric orbit with a period of approximately 7h 45m. Its companion has not yet been identified with certainty, but must be a compact object of mass comparable to that of the ...
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Vainshtein mechanism in binary pulsars
Physical Review D, 2013 minor revisions to match published version in ...
de Rham, Claudia +2 more
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Trompe L'Oeil 'binary' pulsars
The Astrophysical Journal, 1990 A freely precessing pulsar produces pulse phase residuals which can mimic those of a pulsar in a binary orbit. In particular, discrete sets of phase residuals due to precessional motion of an isolated pulsar are sampled; it is shown that this data is well fit by residuals from a binary pulsar in a sufficiently tight orbit.
Robert W. Nelson +2 more
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Binary-Binary Interactions and the Formation of the PSR B1620-26 Triple System in M4 [PDF]
, 1994 The hierarchical triple system containing the millisecond pulsar PSR B1620-26 in M4 is the first triple star system ever detected in a globular cluster. Such systems should form in globular clusters as a result of dynamical interactions between binaries.
Hut, P., McMillan, S., Rasio, F. A.
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Relativistic Binary Pulsars with Black Hole Companions [PDF]
The Astrophysical Journal, 2005 Binaries containing a stellar-mass black hole and a recycled radio pulsar have so far eluded detection. We present a focused investigation of the formation and evolution of these systems in the Galactic disk, highlighting the factors that limit their numbers and the reasons why they may be extremely rare.
Pfahl, E, Podsiadlowski, P, Rappaport, S
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A Radio Pulsar/X-ray Binary Link [PDF]
Science, 2009 From X-ray Binary to Pulsar Pulsars with millisecond rotational periods are thought to originate from neutron stars in low-mass x-ray binaries that had their spin frequencies increased by long-lasting mass transfer from their companion stars. Using data from a radio pulsar survey, Archibald
Archibald, A.M. +17 more
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Physical Review X, 2017 Pulsar timing and laser-interferometer gravitational-wave (GW) detectors are superb laboratories to study gravity theories in the strong-field regime. Here, we combine these tools to test the mono-scalar-tensor theory of Damour and Esposito-Farèse (DEF),
Lijing Shao +4 more
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