The Kick Velocity Distribution of Isolated Neutron Stars
Neutron stars (NSs) are thought to receive natal kicks at their formation in supernovae. In order to investigate the magnitude of these kicks, we analyze the proper motions and distance estimates—through either parallax or dispersion measures—of young ...
Paul Disberg, Ilya Mandel
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Expansion of Accreting Main-sequence Stars during Rapid Mass Transfer
Accreting main-sequence stars expand significantly when the mass accretion timescale is much shorter than their thermal timescales. This occurs during mass transfer from an evolved giant star onto a main-sequence companion in a binary system and is an ...
Mike Y. M. Lau +3 more
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Preparing for gravitational wave astronomy : a verification of the GEO 600 detection chain by generation, injection, and extraction of continuous signals [PDF]
U. Weiland
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Perspectives for multi-messenger astronomy with the next generation of\n gravitational-wave detectors and high-energy satellites [PDF]
S. Ronchini +8 more
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Choosing Suitable Noise Models for Nanohertz Gravitational-wave Astrophysics
Accurately estimating the parameters of the nanohertz gravitational-wave background is essential for understanding its origin. The background is typically modeled with a power-law spectrum, parameterized with an amplitude A , which describes its ...
Valentina Di Marco +4 more
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The promises of gravitational-wave astronomy. [PDF]
Martin IW +3 more
europepmc +1 more source
Special Lecture “KAGRA and Gravitational-wave Astronomy”
Hiroshi Daimon
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New physics and astronomy with the new gravitational-wave observatories [PDF]
Scott A. Hughes +3 more
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The Promise of Low-Frequency Gravitational Wave Astronomy [PDF]
T. Prince
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