Results 141 to 150 of about 777,035 (267)

COBIPULSE: A Systematic Search for Compact Binary Millisecond Pulsars

The Astrophysical Journal
We report here the results obtained from a systematic optical photometric survey aimed at finding new compact binary millisecond pulsars (also known as “spiders”): the COmpact BInary PULsar SEarch. We acquired multiband optical images over 1 yr around 33
Marco Turchetta, Manuel Linares, Karri Koljonen, Jorge Casares, Paulo A. Miles-Páez, Pablo Rodríguez-Gil, Tariq Shahbaz, Jordan A. Simpson   +7 more
doaj   +1 more source

Neutron star mass estimates from gamma-ray eclipses in spider millisecond pulsar binaries. [PDF]

Nat Astron, 2023
Clark CJ, Kerr M, Barr ED, Bhattacharyya B, Breton RP, Bruel P, Camilo F, Chen W, Cognard I, Cromartie HT, Deneva J, Dhillon VS, Guillemot L, Kennedy MR, Kramer M, Lyne AG, Sánchez DM, Nieder L, Phillips C, Ransom SM, Ray PS, Roberts MSE, Roy J, Smith DA, Spiewak R, Stappers BW, Tabassum S, Theureau G, Voisin G.   +28 more
europepmc   +1 more source

Binary Pulsars: Observations and Implications [PDF]

, 1987
J. H. Taylor
openalex   +1 more source

Revisiting the double-binary-pulsar probe of nondynamical Chern-Simons gravity

, 2011
One of the popular modifications to the theory of general relativity is nondynamical Chern-Simons (CS) gravity, in which the metric is coupled to an externally prescribed scalar field.
Yacine Ali-Haïmoud
semanticscholar   +1 more source

No tension between assembly models of super massive black hole binaries and pulsar observations

Nature Communications, 2018
Pulsar timing arrays enable the search for the isotropic gravitational-wave (GW) background originating from super massive black hole binary populations, but impose a stringent upper limit on the GW characteristic amplitude.
Hannah Middleton, Siyuan Chen, Walter Del Pozzo, Alberto Sesana, Alberto Vecchio   +4 more
doaj   +1 more source

Further experimental tests of relativistic gravity using the binary pulsar PSR 1913+16

, 1989
Fourteen-year observations of the binary pulsar PSR 1913 + 16 provided data consistent with a straightforward model allowing for the motion of the earth, special and general relativistic effects within the solar system, dispersive propagation in the ...
Joseph H. Taylor, J. Weisberg
semanticscholar   +1 more source

Thirty-five Years of Timing of M53A with Arecibo and FAST

The Astrophysical Journal Letters
PSR B1310+18A is a 33 ms binary pulsar in a 256 day, low eccentricity orbit with a low-mass companion located in NGC 5024 (M53). In this Letter, we present the first phase-coherent timing solution for this pulsar (designated as M53A) derived from a 35 yr
Yujie Lian, P. C. C. Freire, Shuo Cao, Mario Cadelano, Cristina Pallanca, Zhichen Pan, Haiyan Zhang, Baoda Li, Lei Qian   +8 more
doaj   +1 more source

Verification of f(R)-gravity in binary pulsars

EPJ Web of Conferences, 2016
We develop the parameterized post-Keplerian approach for class of analytic f (R)-gravity models. Using the double binary pulsar system PSR J0737-3039 data we obtain restrictions on the parameters of this class of f (R)-models and show that f (R)-gravity ...
Dyadina Polina, Alexeyev Stanislav, Capozziello Salvatore, De Laurentis Mariafelicia   +3 more
doaj   +1 more source

Strongly interacting matter exhibits deconfined behavior in massive neutron stars. [PDF]

Nat Commun, 2023
Annala E, Gorda T, Hirvonen J, Komoltsev O, Kurkela A, Nättilä J, Vuorinen A.   +6 more
europepmc   +1 more source

Gravitational radiation and steady-state distribution of binary orbits: application to high-mass binary pulsars [PDF]

, 1994
J. Buitrago, C. Moreno-Garrido, E. Mediavilla   +2 more
openalex   +1 more source