Results 81 to 90 of about 480,915 (121)
European Physical Journal C: Particles and FieldsOrdinary matter coupled to light weakly interacting bosons can lead to the formation of a macroscopic bosonic field in the vicinity of large matter concentrations such as ordinary or neutron stars.
Arturo de Giorgi, Joerg Jaeckel
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IMAGES OF GRAVITATIONAL AND MAGNETIC PHENOMENA DERIVED FROM TWO-DIMENSIONAL BACK-PROJECTION DOPPLER TOMOGRAPHY OF INTERACTING BINARY STARS [PDF]
, 2014 Mercedes T. Richards +3 more
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Mass-transferring binary stars as progenitors of interacting hydrogen-free supernovae [PDF]
Andrea Ercolino +3 more
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AGB winds in interacting binary stars [PDF]
, 2020 Luis C. Bermúdez-Bustamante +3 more
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The Imprint of Dark Matter on the Galactic Acceleration Field
The Astrophysical JournalMeasurements of the accelerations of stars enabled by time-series extreme-precision spectroscopic observations, pulsar timing, and eclipsing binary stars in the solar neighborhood offer insights into the mass distribution of the Milky Way that do not ...
Arpit Arora +8 more
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Observational constraints on massive binaries [PDF]
arXivBinary interactions are commonplace among massive stars, giving rise observed phenomena such as X-ray binaries, stripped stars & supernovae, and gravitational-wave sources. The multiplicity properties of massive stars thus represent a fundamental observable to calibrate, test, and benchmark models of single-star and binary evolution.
arxiv
To Be or Not To Be: The Role of Rotation in Modeling Galactic Be X-Ray Binaries
The Astrophysical JournalBe X-ray binaries (Be-XRBs) are one of the largest subclasses of high-mass X-ray binaries, comprised of a rapidly rotating Be star and neutron star companion in an eccentric orbit, intermittently accreting material from a decretion disk around the donor.
Kyle Akira Rocha +13 more
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Transmuted gravity wave signals from primordial black holes
Physics Letters B, 2018 Primordial black holes (PBHs) interacting with stars in binaries lead to a new class of gravity wave signatures that we explore. A small 10−16–10−7M⊙ PBH captured by a neutron star or a white dwarf will eventually consume the host.
Volodymyr Takhistov
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What Can We Learn about the Unstable Equation-of-state Branch from Neutron Star Mergers?
The Astrophysical Journal LettersThe equation of state (EOS) of dense strongly interacting matter can be probed by astrophysical observations of neutron stars (NS), such as X-ray detections of pulsars or the measurement of the tidal deformability of NSs during the inspiral stage of NS ...
Maximiliano Ujevic +4 more
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