يعرض 1 - 7 نتائج من 7 نتيجة بحث عن '"individual: Messier 31 [galaxies]"', وقت الاستعلام: 0.93s تنقيح النتائج
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    مصطلحات موضوعية: statistics [galaxies], instruments [space vehicles], galaxies [submillimeter], cosmic background radiation, general [X-rays], Astrophysics::Solar and Stellar Astrophysics, clusters: general [galaxies], submillimeter, dark ages, general [radiation mechanisms], relativistic processes, astro-ph.HE, theory [cosmology], general [ISM], extinction, supernova remnants [ISM], Astrophysics::Instrumentation and Methods for Astrophysics, ISM [infrared], observations [cosmology], bubbles [ISM], ISM - dust, observations, clusters: intracluster medium [galaxies], active [galaxies], structure [galaxies], astro-ph.CO, reionization, Astrophysics::Earth and Planetary Astrophysics, dust, large-scale structure of Universe, star formation [galaxies], disk [Galaxy], clouds [ISM], local insterstellar matter, high-redshift [galaxies], Astronomical and Space Sciences, Astrophysics::High Energy Astrophysical Phenomena, astro-ph.GA, statistical [methods], first stars, individual: Messier 31 [galaxies], ISM [radio continuum], Astrophysics::Cosmology and Extragalactic Astrophysics, Astronomy & Astrophysics, Affordable and Clean Energy, ISM [gamma rays], cosmic rays, surveys, weak [gravitational lensing], diffuse background [infrared], atomic data, data analysis [methods], reference systems, general [planets and satellites], cosmological parameters, ISM [submillimeter], general [infrared], general [Galaxy], evolution [galaxies], Astrophysics::Galaxy Astrophysics, nucleus [Galaxy], polarization, detectors [instrumentation], ISM [galaxies], turbulence, magnetic fields [ISM], clusters: individual: Virgo [galaxies], general [submillimeter], galaxies [radio continuum], diffuse radiation, astro-ph.EP, structure [ISM], magnetohydrodynamics, cosmology, catalogs, general [galaxies], astro-ph.IM

    وصف الملف: application/pdf

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    المساهمون: University of Oslo, University of Cambridge, Université Paris-Sud, International School for Advanced Studies, University of Bologna, CNRS, CSIC, University of Padova, Institut d 'Astrophysique de Paris, University of Milan, University of Oviedo, University of Toronto, Lawrence Berkeley National Laboratory, Observatoire de Paris, University of Ferrara, Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna, University of Oxford, University of Sussex, University of KwaZulu-Natal, University of Southern California, Université Grenoble Alpes, California Institute of Technology, Sapienza University of Rome, Astronomical Observatory of Padua, University of Manchester, Imperial College London, European Space Astronomy Centre, University College London, Max Planck Institute for Astrophysics, African Institute for Mathematical Sciences, Jodrell Bank Centre for Astrophysics, Topological Quantum Fluids, Department of Applied Physics, Aalto-yliopisto, Aalto University, Cardiff University, Metsähovi Radio Observatory, University of Helsinki, Université de Toulouse, Universidad de Cantabria, Instituto Nationale di Fisica Nucleare, University of Granada, Pierre and Marie Curie University, Istituto Nazionale Astrofisica - Italy, University of California Berkeley, Telecom ParisTech, University of Paris Diderot, Princeton University, Niels Bohr Institute, University of Copenhagen, Department of Radio Science and Engineering, Université Paris Diderot, Kavli Institute for Cosmology Cambridge, Université Fédérale Toulouse Midi-Pyrénées, Università degli Studi di Milano, Nicolaus Copernicus Astronomical Center, INAF/IASF Bologna, Niels Bohr Institute, INAF, Osservatorio Astronomico di Padova, Ludwig Maximilian University of Munich, INAF/IASF Milano, European Space Agency - ESA

    وصف الملف: application/pdf

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    وصف الملف: application/pdf

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