Journal•ISSN: 1384-1076
New Astronomy
Elsevier BV
About: New Astronomy is an academic journal published by Elsevier BV. The journal publishes majorly in the area(s): Light curve & Stars. It has an ISSN identifier of 1384-1076. Over the lifetime, 2117 publications have been published receiving 40646 citations.
Topics: Light curve, Stars, Galaxy, Orbital period, Contact binary
Papers published on a yearly basis
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TL;DR: The newly written code GADGET is described, which is suitable both for cosmological simulations of structure formation and for the simulation of interacting galaxies, and a parallel version that has been designed to run on massively parallel supercomputers with distributed memory.
1,588 citations
Pontifical Catholic University of Chile1, University of Hertfordshire2, Queen Mary University of London3, European Southern Observatory4, National University of Cordoba5, University of Michigan6, University of La Serena7, University of Florida8, University of São Paulo9, Space Telescope Science Institute10, Universidade Federal do Rio Grande do Sul11, Valparaiso University12, University of Chile13, Chinese Academy of Sciences14, University of Sheffield15, Hungarian Academy of Sciences16, Imperial College London17, National University of La Plata18, University of Concepción19, Max Planck Society20, University of Cambridge21, University of Manchester22, Spanish National Research Council23, University of Southampton24, INAF25, Rochester Institute of Technology26, European Space Research and Technology Centre27, University of Padua28, Andrés Bello National University29, University of Leicester30, Hartebeesthoek Radio Astronomy Observatory31, University of Kent32
TL;DR: In this article, the authors proposed a method to solve the problem of single-input single-output (SISO) communication in the context of artificial neural networks (ANNs).
927 citations
TL;DR: The Gasoline as discussed by the authors is an extension of the Pkdgrav parallel N-body code using smoothed particle hydrodynamics, which is used to simulate galaxy clusters, galaxy formation and gas-giant planets.
722 citations
TL;DR: In this paper, the chemistry and cooling behavior of low-density (n ≲ 10 4 cm −3 ) primordial gas and devised a model which involves 19 collisional and 9 radiative processes and is applicable for temperatures in the range 1 K T 8 K.
568 citations
TL;DR: In this paper, it was shown that if protons are accelerated at the maximum possible rate, i.e. tacc=η(rg/c) with so-called gyro-factor η∼1, the synchrotron cooling of protons could not only dominate over other radiative and non-radiative losses, but also provide good fits (within uncertainties introduced by extragalactic γ-ray extinction) to the γradiation of two firmly established TeV blazars.
488 citations