Results 31 to 40 of about 1,314,919 (318)
Properties of the Binary Neutron Star Merger GW170817 [PDF]
, 2018 On August 17, 2017, the Advanced LIGO and Advanced Virgo gravitational-wave detectors observed a low-mass compact binary inspiral. The initial sky localization of the source of the gravitational-wave signal, GW170817, allowed electromagnetic ...
The Ligo Scientific Collaboration +499 more
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Journal of Pharmaceutical Analysis, 2023 Peptide-based therapeutics are increasingly pushing to the forefront of biomedicine with their promise of high specificity and low toxicity. Although noncanonical residues can always be used, employing only the natural 20 residues restricts the chemical ...
Sarfraz Ahmad +2 more
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Binary star formation and the outflows from their discs [PDF]
, 2017 We carry out magnetohydrodynamical simulations with FLASH of the formation of a single, a tight binary ($a\sim$2.5 AU) and a wide binary star ($a\sim$45 AU).
R. Kuruwita, C. Federrath, M. Ireland
semanticscholar +1 more source
Iraqi Journal of Physics, 2019 In this research the change in the distance of the two stars in two binary star systems (13.6+8)M8and (13+10)M8 was studied, through the calculations the value (rate of mass transfer) of the two phases of dynamical stages of mass which are mass loss ...
Mohammed R. Abdulameer
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K2-136: A Hyades Binary Star with a Neptune-sized Planet [PDF]
, 2017 We report the discovery of a Neptune-size planet (Rp = 3.0 Re) in the Hyades Cluster. The host star is in a binary system, comprising a K5V star and M7/8V star with a projected separation of 40 AU.
D. Ciardi +16 more
semanticscholar +1 more source
The Astronomical Journal, 2023 In this study, we continue our project to search for unresolved binary and multiple systems in open clusters exploiting the photometric diagram (H–W2)–W1 versus W2–(BP–K) first introduced in Malofeeva et al. In particular, here we estimate the binary and
Alina A. Malofeeva +3 more
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PRELIMINARY RESULTS OF MODELING OF LIGHT CURVES OF WW AND
Odessa Astronomical Publications, 2017 In this work we present the preliminary results of modeling of Olson’s lybv light curves of an Algol-type binary WW And. A model of a binary star containing an accretion disk around the primary star is deployed.
S. Zola
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Binary Neutron Star Mergers After GW170817
Frontiers in Astronomy and Space Sciences, 2020 The first combined detection of gravitational waves and electromagnetic signals from a binary neutron star (BNS) merger in August 2017 (an event named GW170817) represents a major landmark in the ongoing investigation of these extraordinary systems.
Riccardo Ciolfi, Riccardo Ciolfi
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Properties of Binary Systems in a One-dimensional Approximation
The Astrophysical Journal, 2023 Evolutionary calculations for stars in close binary systems are in high demand to obtain better constraints on gravitational-wave source progenitors, understand transient events from stellar interactions, and more.
Ali Pourmand, Natalia Ivanova
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Constraints on the speed of sound of dense nuclear matter through the tidal deformability of neutron stars [PDF]
EPJ Web of Conferences, 2021 One of the greatest interest and open problems in nuclear physics is the upper limit of the speed of sound in dense nuclear matter. Neutron stars, both in isolated and binary system cases, constitute a very promising natural laboratory for studying this ...
Kanakis-Pegios Alkiviadis +2 more
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