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Astrophysical Journal, ISSN 0004-637X, 09/2016, Volume 829, Issue 1, p. 55
Journal Article
Astrophysical Journal, ISSN 0004-637X, 10/2015, Volume 812, Issue 2, p. 143
To understand the nature of supernovae and neutron star (NS) formation, as well as binary stellar evolution and their interactions, it is important to probe... 
pulsars: individual (J0453+1559) | pulsars: general | gravitational waves | J1906+0746 | GENERAL-RELATIVITY | GRAVITY | MILLISECOND PULSARS | PSR-1913+16 | MOTION | YOUNG | PSR J1756-2251 | ASTRONOMY & ASTROPHYSICS | RELATIVISTIC BINARY PULSAR | WHITE-DWARF COMPANIONS | Orbitals | Neutron stars | Supernovae | Searching | Progenitors (astrophysics) | Pulsars | Formations | Companion stars
Journal Article
Astrophysical Journal, ISSN 0004-637X, 08/2018, Volume 862, Issue 2, p. 139
Using the Very Long Baseline Array, we have made astrometric observations of the binary pulsar B1913+16 spanning an 18-month period in 2014-2015. From these... 
techniques: high angular resolution | gravitation | pulsars: individual (PSR B1913+16) | astrometry | stars: neutron | NEUTRON-STAR SYSTEMS | PARALLAXES | PROPER MOTIONS | BIAS | ASTRONOMY & ASTROPHYSICS | BINARY PULSAR PSR-1913+16
Journal Article
Astrophysical Journal, ISSN 0004-637X, 01/1991, Volume 366, Issue 2, pp. 501 - 511
We reexamine the theoretical significance of the raw observational parameter called the "rate of orbital period change," P(b)obs, of the binary pulsar PSR 1913... 
Gravitation | Stars: binaries | Stars: stellar dynamics | Pulsars | Relativity | SYSTEM | ROTATION | PULSARS | DISTANCE | ARRIVAL-TIME ANALYSIS | GRAVITATIONAL-RADIATION | FORMULA | PSR 1913+16 | VARIABILITY | RELATIVISTIC CELESTIAL MECHANICS | ASTRONOMY & ASTROPHYSICS | STARS BINARIES | GRAVITATION | STARS STELLAR DYNAMICS | MILKY-WAY | RELATIVITY
Journal Article
Astrophysical Journal Letters, ISSN 2041-8205, 10/2017, Volume 848
On 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational... 
OPTICAL AFTERGLOWS | NEARBY SUPERNOVA RATES | GRAVITATIONAL-WAVES | PULSAR PSR-1913+16 | COMPACT OBJECTS | gravitational waves | RADIO TELESCOPE | CLOSE BINARIES | GAMMA-RAY BURSTS | stars: neutron | RELATIVISTIC GRAVITY | BLACK-HOLES
Journal Article
Classical and Quantum Gravity, ISSN 0264-9381, 12/2012, Volume 29, Issue 24, p. 245004
Observations of pulsar timing provide strong constraints on scalar-tensor theories of gravity, but these constraints are traditionally quoted as limits on the... 
SYSTEM | STRONG-FIELD TESTS | RELATIVISTIC CELESTIAL MECHANICS | GENERAL-RELATIVITY | PHYSICS, MULTIDISCIPLINARY | ASTRONOMY & ASTROPHYSICS | PHYSICS | BINARY-PULSAR | MACHS PRINCIPLE | DISCOVERY | PSR-1913+16 | PHYSICS, PARTICLES & FIELDS
Journal Article
Reviews of Modern Physics, ISSN 0034-6861, 07/1994, Volume 66, Issue 3, pp. 711 - 719
Journal Article
Astrophysical Journal, ISSN 0004-637X, 07/1992, Volume 393, Issue 2, pp. L59 - L61
According to some metric theories of gravity, the center of mass of a binary system may be "self-accelerated" in the direction of the periastron of the orbit... 
Binaries: general | Gravitation | GRAVITATION | BINARIES, GENERAL | ASTRONOMY & ASTROPHYSICS | RELATIVISTIC GRAVITY | PULSARS, INDIVIDUAL, PSR-1913+16
Journal Article
Classical and Quantum Gravity, ISSN 0264-9381, 12/1993, Volume 10, Issue 12, pp. 2699 - 2721
Gravitational wave tails are produced by back-scattering of the outgoing gravitational radiation (emitted by an isolated system) off the curved spacetime... 
POST-NEWTONIAN GENERATION | RELATIVISTIC CELESTIAL MECHANICS | COALESCING BINARIES | PULSAR PSR-1913+16 | COMPACT OBJECTS | PHYSICS | (POST)5/2-NEWTONIAN ORDER | RADIATION | EQUATION | SCALAR | NONSPHERICAL PERTURBATIONS
Journal Article
Astrophysical Journal, ISSN 0004-637X, 08/1996, Volume 467, Issue 2, pp. L93 - L95
The proper motion of a binary pulsar gradually changes the apparent geometrical orientation of its orbital plane. Consequently, the derived values of the... 
Gravitation | Stars: binaries | Stars: fundamental parameters | Stars: neutron | Relativity | TESTS | pulsars, individual (B1534+12, B1855+09, B1913+16) | gravitation | stars, fundamental parameters | ASTRONOMY & ASTROPHYSICS | stars, neutron | RELATIVISTIC GRAVITY | relativity stars, binaries | PSR-1913+16
Journal Article
by Lo, C.Y
Astrophysical Journal, ISSN 0004-637X, 12/1995, Volume 455, Issue 2, pp. 421 - 428
Einstein's radiation formula is supported by the Taylor-Hulse experiment, but its derivation is not self-consistent. Furthermore, as discovered by Einstein,... 
Gravitation | Radiation mechanisms: nonthermal | Relativity | RADIATION MECHANISMS, NONTHERMAL | GENERAL-RELATIVITY | FIELD-THEORY | ASTRONOMY & ASTROPHYSICS | GRAVITATION | PULSAR | GRAVITATIONAL-RADIATION | RELATIVITY | PSR-1913+16
Journal Article
Journal of the Physical Society of Japan, ISSN 0031-9015, 1997, Volume 66, Issue 4, pp. 1225 - 1228
We briefly review possible systematic limitations to inferredGeneral Relativity tests in binary pulsar systems, then proposea new mechanism whereby orbital... 
binary pulsar | neutrino | general relativity | dissipation | Binary pulsar | Neutrino | Dissipation | General relativity | PHYSICS, MULTIDISCIPLINARY | PSR-1913+16
Journal Article
Astrophysical Journal, ISSN 0004-637X, 1996, Volume 462, Issue 1, pp. 287 - 288
Journal Article
PHYSICAL REVIEW D, ISSN 0556-2821, 12/1998, Volume 5812, Issue 12, pp. 4002 - 4002
We derive the gravitational field and equations of motion of compact binary systems up to the 5/2 post-Newtonian approximation of general relativity (where... 
GENERAL-RELATIVITY | APPROXIMATION | PULSAR PSR-1913+16 | ENERGY-LOSS | WAVE-FORM | CIRCULAR ORBIT | RADIATION-REACTION | BLACK-HOLE | POINT MASSES | CANONICAL FORMALISM | PHYSICS, PARTICLES & FIELDS
Journal Article
Journal of Astrophysics and Astronomy, ISSN 0250-6335, 06/1995, Volume 16, Issue 2, pp. 307 - 325
Journal Article
PHYSICAL REVIEW D, ISSN 2470-0010, 10/1997, Volume 56, Issue 8, pp. 4455 - 4469
Fundamental limits on the energy density Omega(g) of the ultralow-frequency primordial gravitational wave background (GWB) radiation which can be obtained from... 
TESTS | GENERAL-RELATIVITY | MILLISECOND PULSAR | CRAB PULSAR | FLUCTUATIONS | ASTRONOMY & ASTROPHYSICS | TIMING NOISE | RADIATION-REACTION | RELATIVISTIC GRAVITY | UPPER LIMITS | PSR-1913+16 | PHYSICS, PARTICLES & FIELDS
Journal Article
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