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Radio Galaxies at TeV Energies

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Spectral Energy Distribution Of Galaxies - Sed 2011 (Iau S28

Recent observational developments are providing the first truly panchromatic view of galaxies, extending from the radio to TeV gamma rays;

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Cherenkov Reflections

, mainly in the TeV energy regime but also where relevant at PeV energies. The narrative traces the contributions of many important participants;

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Clusters of Galaxies & Extragalactic Radio Sources

Clusters of Galaxies & Extragalactic Radio Sources;

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Plasma Astrophysics and Cosmology

, in stars, galaxies, and clusters of galaxies, and throughout the observable universe. Plasma astrophysics and cosmology, as a unified discipline;

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The Multiwavelength Atlas of Galaxies

Since the radio signature of our own Milky Way was detected in 1931, galaxies have been observed from ultra-high energy gamma rays to long;

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The Nearest Active Galaxies

include circumnuclear populations in nearby AGN, the starburst scenario for radio emission in active galaxies, radiation from arbitrarily shaped;

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Black Holes from the Stars to Galaxies--Across the Range of Masses

overwhelming evidence in favour of the presence of supermassive black holes at the centre of galaxies, including the Milky Way; of stellar-mass black;

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Clusters and Superclusters of Galaxies

Clusters and superclusters of galaxies are the largest objects in the Universe and are the subject of intense observational study at a;

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Galaxies In 3D Across The Universe IAU S

surveys aiming at a full census of galaxies across the local Universe. Reaching out to the limits of the Universe, the evolution of spatially;

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Radio-Frequency And Elf Electromagnetic Energies

Tailored especially for the working health professional, Radio Frequency and ELF Electrogmagnetic Energies is a practical guide to;

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Physics of the Plasma Universe

, and intergalactic space; in stars, galaxies, and clusters of galaxies, and throughout the observable universe. Physics of the Plasma Universe;

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An Introduction to Active Galactic Nuclei

How can we test if a supermassive black hole lies at the heart of every active galactic nucleus? What are LINERS, BL Lacs, N galaxies;

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Cambridge Astrophysics

of galaxies. In our universe, clusters of galaxies are the largest organised structures. Typically they comprise hundreds of galaxies moving through a;

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Revealing The Heart Of The Galaxy

luminous objects in the Universe - quasars and radio galaxies - are powered by massive black holes at their hearts. But how did black holes emerge;

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Galaxies at High Redshift

methods suited to the study of distant galaxies. This volume contains the lectures delivered at the XI Canary Islands Winter School;

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The Most Interesting Galaxies in the Universe

some having supermassive black holes at their core, others are powerful radio sources, a very few are relatively nearby and even visible to the;

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Become One

part. In the process of becoming one these galaxies will continue to pull and tug at one another for several billion years, before they;

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Galaxies at High Redshift

methods suited to the study of distant galaxies. This volume contains the lectures delivered at the XI Canary Islands Winter School;

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Molecular Gas, Dust, And Star Formation In Galaxies (Iau S29

Our knowledge of the molecular gas content in galaxies has advanced rapidly in the past decade with systematic surveys from ground-based;

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Warped Disks and Inclined Rings around Galaxies

galaxies with inclined HI rings or unusual 'tails'. This book is a record of a meeting which was held at the University of Pittsburgh. It provided;

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Warped Disks and Inclined Rings around Galaxies

galaxies with inclined HI rings or unusual 'tails'. This book is a record of a meeting which was held at the University of Pittsburgh. It provided;

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Measurement of Higgs Boson Production Cross Sections in the Diphoton Channel

-proton collision data at a center-of-mass energy s = 13 TeV recorded by the ATLAS experiment at the Large Hadron Collider (LHC). The collected;

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Wounded Galaxies Tap At Window. Cyclobe, CD

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Particle Interactions at Very High Energies

Particle Interactions at Very High Energies is een boek van Francis Halzen;

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The Stellar Populations of Galaxies

One approach to learning about stellar populations is to study them at three different levels of resolution. First in our own galaxy;

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Isospin Physics in Heavy-Ion Collisions At Intermediate Energies

Isospin Physics in Heavy-Ion Collisions At Intermediate Energies;

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