Results 11 to 20 of about 8,111 (268)
Binary–binary scattering in the secular limit [PDF]
Monthly Notices of the Royal Astronomical Society, 2020 ABSTRACT Binary–binary interactions are important in a number of astrophysical contexts including dense stellar systems such as globular clusters. Although less frequent than binary–single encounters, binary–binary interactions lead to a much richer range of possibilities such as the formation of stable triple systems.
Johan Samsing, Adrian S Hamers
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Variable binaries and variables in binaries in the Binary star DataBase [PDF]
Research in Astronomy and Astrophysics, 2019 Abstract The Binary star DataBase (BDB, http://bdb.inasan.ru ) combines data from catalogs of binary and multiple stars of all observational types. There is a number of ways for variable stars to form or to be a part of binary or multiple systems.
Kovaleva, D., Malkov, O., Kaygorodov, P.
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Binary consensus through binary communication [PDF]
53rd IEEE Conference on Decision and Control, 2014 The problem of binary consensus for an undirected, synchronous, fixed topology network through noiseless, binary communication is the focus of this paper. We propose a binary consensus protocol that guarantees network convergence to the initial network majority via binary communication among one-hop neighbors.
George, Jemin, Swami, Ananthram
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AppliedMath, 2022 This paper investigates the behavior of rotating binaries. A rotation by r digits to the left of a binary number B exhibits in particular cases the divisibility l∣N1(B)·r+1, where l is the bit-length of B and N1(B) is the Hamming weight of B, that is the number of ones in B. The integer r is called the left-rotational distance.
Anant Gupta +5 more
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Binary Be Stars and Be Binaries [PDF]
Symposium - International Astronomical Union, 1992 Two hypotheses have been put forward for the rôle of binarity in Be stars: (1) All Be stars are interacting binaries. (2) Roughly one-half of the observed Be stars are post-mass exchange binaries with compact companions. Contrary to (1), (2) does not attempt to explain also the existence of disks in Be stars.
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Open Astronomy, 2017 Evolved stars with a helium core can be formed by non-conservative mass exchange interaction with a companion or by strong mass loss. Their masses are smaller than 0.5 M⊙. In the database of the Sloan Digital Sky Survey (SDSS), there are several thousand
Pelisoli Ingrid +2 more
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Binary autoencoder with random binary weights
CoRR, 2020 Here is presented an analysis of an autoencoder with binary activations $\{0, 1\}$ and binary $\{0, 1\}$ random weights. Such set up puts this model at the intersection of different fields: neuroscience, information theory, sparse coding, and machine learning.
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Stellar collisions during binary-binary and binary-single star interactions [PDF]
Monthly Notices of the Royal Astronomical Society, 2004 Accepted for publication in MNRAS; 29 pages, 22 figures, 7 ...
Fregeau, J.M. +3 more
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Beyond binaries and before becoming: Reconsidering resistance in UK higher education
PRISM, 2023 Drawing from the tensions within non-representational and human practice perspectives on affect, this paper continues the task of re-conceptualising academic-level resistance in the context of UK higher education. Such re-conceptualisation is underpinned
Mollie Baker
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The Asymptotic Number of Binary Codes and Binary Matroids [PDF]
SIAM Journal on Discrete Mathematics, 2005 12 ...
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