scholarly article | Q13442814 |
P819 | ADS bibcode | 1994Natur.369..127L |
P6179 | Dimensions Publication ID | 1007770185 |
P356 | DOI | 10.1038/369127A0 |
P2093 | author name string | A. G. Lyne | |
D. R Lorimer | |||
P2860 | cites work | Spatial distribution of γ-ray bursts observed by BATSE | Q54197231 |
Pulsar distances and the galactic distribution of free electrons | Q55952099 | ||
Timing and scintillation observations of the fast pulsar in CTB80 | Q58979387 | ||
Gamma-ray bursts from high-velocity neutron stars | Q59068690 | ||
Interstellar scintillation and pulsar velocities | Q59088460 | ||
Formation and evolution of binary and millisecond radio pulsars | Q68246071 | ||
Pulsar velocities and the scaleheight of scattering in the Galaxy | Q68249627 | ||
Pulsar statistics : the birthrate and initial spin periods of radio pulsars | Q68255941 | ||
Positions and proper motions of pulsars | Q68261514 | ||
New determinations of the proper motions of 44 pulsars | Q68473942 | ||
The proper motions of 26 pulsars | Q68559730 | ||
Can we observe accreting, isolated neutron stars ? | Q68794815 | ||
Associating young pulsars and supernova remnants : PSR 1610-50 and the case for high-velocity pulsars | Q68797021 | ||
The proper motion of the Vela pulsar | Q68833425 | ||
Pulsar populations and their evolution | Q68836774 | ||
Neutron stars and millisecond pulsars from accretion-induced collapse in globular clusters | Q68836913 | ||
P433 | issue | 6476 | |
P407 | language of work or name | English | Q1860 |
P304 | page(s) | 127–131 | |
P577 | publication date | 1994-05-01 | |
P1433 | published in | Nature | Q180445 |
P1476 | title | High birth velocities of radio pulsars | |
P478 | volume | 369 |
Q57808506 | A large age for the pulsar B1757-24 from an upper limit on its proper motion |
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Q30835875 | Binary and Millisecond Pulsars |
Q39127321 | Binary and Millisecond Pulsars at the New Millennium |
Q68537157 | Cooling flows or warming rays? |
Q68670458 | Discovery of a 7 second anomalous X-ray pulsar in the distant Milky Way |
Q59098848 | Evidence from a processing pulsar orbit for a neutron-star birth kick |
Q21563857 | Experimental astrophysics with high power lasers and Z pinches |
Q68786059 | First LIGO events: binary black holes mergings |
Q56489546 | Formation of the Black Hole in Nova Scorpii |
Q29027920 | Gamma-ray bursts and the fireball model |
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Q57518886 | IKT 16: a composite supernova remnant in the Small Magellanic Cloud |
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Q57854334 | Limits on intermediate-mass black holes in six Galactic globular clusters with integral-field spectroscopy |
Q56555361 | Maximum speed of hypervelocity stars ejected from binaries |
Q68367856 | Neutrinos and supernova theory |
Q63640396 | Neutron stars accreting the ISM: Are they fast or slow objects? |
Q68519154 | Neutron stars: how pulsars get their spins |
Q56573219 | Nucleosynthesis in neutron-rich ejecta from quark-novae |
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Q68841027 | Origin and possible birthplace of the extreme runaway star HIP 60350 |
Q68508882 | Population synthesis of pulsars: Magnetic field effects |
Q68370761 | Pulsar recoil by large-scale anisotropies in supernova explosions |
Q59076143 | Supernova explosions in the Universe |
Q37599168 | The Evolution of Compact Binary Star Systems |
Q37598630 | The Evolution of Compact Binary Star Systems. |
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