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ORION NEBULA --- ATLASES --- Orion Nebula.
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Supernova remnants --- Congresses. --- Crab Nebula
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Galaxies --- Interstellar matter --- Molecular clouds --- Stars --- Congresses. --- Formation --- Münch Paniagua, Guido, --- Orion Nebula
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Stars --- Astrophysicists --- Etoiles --- Biography --- Congresses --- Formation --- Congrès --- Draper, Henry, --- Orion Nebula --- Festschrift - Libri Amicorum --- Congrès --- Mammals --- Zoohistology. Zoocytology --- Stars - Formation - Congresses --- Draper, Henry, - 1837-1882 - Congresses --- Orion Nebula - Congresses --- Draper, Henry, - 1837-1882
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52 <063> --- Crab Nebula --- -Pulsating stars --- -Pulsating variable stars --- Pulsating variables --- Variable stars --- Stellar oscillations --- Astronomie. Astrofysica. Ruimteonderzoek. Geodesie--Congressen --- Congresses --- Pulsating stars --- Congresses. --- -Astronomie. Astrofysica. Ruimteonderzoek. Geodesie--Congressen --- Pulsating variable stars
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This book summarizes the gathering of information on and the growing understanding of M33 from the 1920s, when Hubble first determined its true nature, to the 21st century, when the Hubble Telescope probed deeply into its many secrets. With its regular symmetrical spiral structure, and its being not tilted too much and near enough to allow detailed studies of its stars, M33 is well-suited for the study of a typical spiral galaxy. In this work, Paul Hodge places current research on M33 (and similar galaxies) in both historical and global perspectives. The book is written in a language accessible for specialists and non-specialists, for professional and amateur astronomers, for scientists and the curious public and, most importantly, for students. .
Spiral galaxies --- Astronomy & Astrophysics --- Physical Sciences & Mathematics --- Astronomy - General --- Astrophysics --- Spiral galaxies. --- Triangulum Galaxy. --- M 33 (Galaxy) --- M33 (Galaxy) --- NGC 598 (Galaxy) --- NGC598 Galaxy) --- Triangulum Nebula --- Astronomy. --- Astronomy, Astrophysics and Cosmology. --- Local Group (Astronomy) --- Galaxies --- Astrophysics. --- Astronomical physics --- Astronomy --- Cosmic physics --- Physics --- Hubble Space Telescope (Spacecraft) --- Space Telescope (Spacecraft) --- Large Space Telescope (Spacecraft) --- HST
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Mass Spectrometry Basics provides authoritative yet plain-spoken explanations of the basic concepts of this powerful analytical method without elaborate mathematical derivations. The authors describe processes, applications, and the underlying science in a concise manner supported by figures and graphics to further comprehension. The text provides practical approaches to interpreting mass spectral data and step-by-step guides for identifying chemically relevant compounds. Additionally, the authors have included an extensive reference section and a quick guide to each chapter that offers immediate access to key information. This unique reference makes some of the esoteric aspects of this important area of analysis more readily comprehensible to those who deal with analytical instruments but who have not been trained in mass spectrometry. It also serves as a refresher for practicing mass spectroscopists by clarifying principles to afford a better appreciation and application of this technology.
spectrometrie --- Theoretical spectroscopy. Spectroscopic techniques --- fysicochemie --- Spectrometric and optical chemical analysis --- massaspectrometrie --- analytische chemie --- Physicochemistry --- spectrometry --- Mass spectrometry. --- Spectrum Analysis, Mass --- Spectrométrie de masse --- Analyseurs de spectre --- Analyse spectrale --- Festschriften --- Handbooks, manuals, etc. --- Mélanges (Recueils) --- Guides, manuels, etc --- Mass spectrometry --- ionisatie --- plasma --- corona --- ion --- laser --- nebula --- gaschromatografie --- isotoop --- Mass spectra --- Mass spectrograph --- Mass spectroscopy --- Mass spectrum analysis --- Mass (Physics) --- Nuclear spectroscopy --- Spectrum analysis --- Spectrométrie de masse --- Mélanges (Recueils)
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The Andromeda Galaxy - Messier's M31 - has an almost romantic appeal. It is the most distant object and the only extragalactic object that is visible to the unaided human eye. It is also almost a twin of the Milky Way Galaxy and our neighbor in space, now known to be about 2.5 million light-years away. The Andromeda Galaxy and the Rise of Modern Astronomy examines ancient and modern astronomical studies of Andromeda and the galaxy's critical role in the development of the science of astrophysics and our growing knowledge of the universe. At the start of the twentieth century the universe was thought of as a finite cosmos dominated by the Milky Way. The study of Andromeda shattered that image, leading ultimately to the conception of an infinite universe of countless galaxies and vast distances. Even today, M31 is a major source of new astronomical discoveries, and it also remains one of the most popular (and rewarding) celestial objects for amateur astronomers to observe and study. Andromeda was once a popular object of folklore and later became central to our understanding of the universe. For all who are interested in astronomy, the skies, and perhaps even the origins of the universe, The Andromeda Galaxy and the Rise of Modern Astronomy provides a first-of-its-kind accessible, informative, and highly readable account of how the study and observation of this celestial object has driven the development of astronomy from ancient times to the present.
Andromeda galaxy. --- Astronomy -- History. --- Astronomy. --- Astronomy --- Astronomy & Astrophysics --- Physical Sciences & Mathematics --- Astrophysics --- Astronomy - General --- History --- History. --- Andromeda Galaxy. --- Andromeda (Nebula) --- Andromeda Spiral --- M31 (Astronomy) --- NGC224 (Astronomy) --- Physics. --- Observations, Astronomical. --- Astrophysics. --- Astronomy, Observations and Techniques. --- Popular Science in Astronomy. --- History of Science. --- Astrophysics and Astroparticles. --- Observations. --- Local Group (Astronomy) --- Annals --- Auxiliary sciences of history --- Astronomy—Observations. --- Astronomical physics --- Cosmic physics --- Physics --- Astronomical observations --- Observations, Astronomical --- Deep space --- Andromeda --- M31 --- NGC224
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This volume celebrates the 30th anniversary of the first very-high energy (VHE) gamma-ray Source detection: the Crab Nebula, observed by the pioneering ground-based Cherenkov telescope Whipple, at teraelectronvolts (TeV) energies, in 1989. As we entered a new era in TeV astronomy, with the imminent start of operations of the Cherenkov Telescope Array (CTA) and new facilities such as LHAASO and the proposed Southern Wide-Field Gamma-ray Observatory (SWGO), we conceived of this volume as a broad reflection on how far we have evolved in the astrophysics topics that dominated the field of TeV astronomy for much of recent history.In the past two decades, H.E.S.S., MAGIC and VERITAS pushed the field of TeV astronomy, consolidating the field of TeV astrophysics, from few to hundreds of TeV emitters. Today, this is a mature field, covering almost every topic of modern astrophysics. TeV astrophysics is also at the center of the multi-messenger astrophysics revolution, as the extreme photon energies involved provide an effective probe in cosmic-ray acceleration, propagation and interaction, in dark matter and exotic physics searches. The improvement that CTA will carry forward and the fact that CTA will operate as the first open observatory in the field, mean that gamma-ray astronomy is about to enter a new precision and productive era.This book aims to serve as an introduction to the field and its state of the art, presenting a series of authoritative reviews on a broad range of topics in which TeV astronomy provided essential contributions, and where some of the most relevant questions for future research lie.
Research & information: general --- Mathematics & science --- gamma ray astronomy --- imaging atmospheric Cherenkov technique --- TeV gamma-rays --- non-thermal radiation --- keV-TeV cosmic sources --- INTEGRAL legacy data base --- relativistic astrophysics --- gamma rays --- cosmic rays --- interstellar medium --- Milky Way --- galaxies --- radiation mechanisms: non-thermal --- high energy astrophysics --- background radiation --- photon–photon interaction --- pair production --- axion-like particles --- gamma-rays --- IACTs --- intergalactic magnetic fields --- high-energy gamma rays --- electromagnetic cascades --- pevatrons --- Galactic cosmic rays --- PeVatron --- Crab Nebula --- angular resolution --- energy spectral distribution --- γ-ray astronomy --- very-high-energy gamma-ray astrophysics --- astroparticle physics --- imaging atmospheric Cherenkov telescopes --- Quantum Gravity --- Lorentz invariance violation --- time of flight --- modified photon interactions --- very-high-energy gamma-ray astronomy --- open science --- data format --- multi-messenger --- real-time --- high-energy --- alerts --- very-high-energy γ-ray astronomy --- atmospheric Cherenkov telescopes --- source catalogues --- gamma-ray astronomy --- Cherenkov telescopes --- ISM: supernova remnants --- ISM: individual objects—Crab Nebula --- pulsars: general --- radiation mechanisms: nonthermal --- gamma rays: general --- acceleration of particles --- astrophysical plasmas --- MHD --- high-energy gamma-ray astrophysics --- Gamma-ray bursts --- non-thermal emission --- radiative processes --- very-high energy Gamma-rays --- statistical analysis --- likelihood --- bayes --- imaging atmospheric Cherenkov telescope --- IACT --- IACT technology --- very high energy gamma-ray telescope --- ground-based gamma-ray astrophysics --- n/a --- photon-photon interaction --- ISM: individual objects-Crab Nebula
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