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Astroquizzical: Solving the Cosmic Puzzles of Our Planets, Stars, and Galaxies

Exploring the family tree of the cosmos, from humans on Earth to stars and galaxies to the first atoms of the Big Bang; with striking;

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The New Physics

in modern physics. Exploring our universe, from the particles within atoms to the stars making up galaxies, it reveals the vital role invisible;

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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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Fundamentals Of Imaging, The: From Particles To Galaxies

of matter to galaxies that are the constituents of the Universe. Imaging must be thought of in a flexible way as varying from just the detection;

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The Stellar Populations of Galaxies

; secondly from nearby galaxies where stars can still be resolved; and thirdly in remote galaxies in which the stellar population can only be studied;

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From Atoms to Galaxies

From Atoms to Galaxies: A Conceptual Physics Approach to Scientific Awareness teaches heightened scientific acuity as it educates students;

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Dynamics of Galaxies

Our understanding of galaxies, the building blocks of the Universe has advanced significantly in recent years. New observations from ground;

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A Catalogue of Southern Peculiar Galaxies and Associations

This is the largest sample yet compiled of over 6,000 disturbed galaxies: observations of galaxies in collision, galaxies exploding or;

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The Nearest Active Galaxies

Reprinted from Astrophysics and Space Science vol. 205, no. 1 (1993), over 30 articles discuss aspects of some nearby galaxies. The topics;

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The Properties of Star-Forming Galaxies at z~2

relation is primarily driven by the increase in metallicity as gas is converted to stars. The picture that emerges is of galaxies with a broad;

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From Interstellar Clouds to Star-Forming Galaxies (IAU S315)

wide range of scales. Bringing together researchers working on star formation throughout the Universe from nearby clouds to local galaxies to;

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The Intriguing Life of Massive Galaxies (Iau S295)

challenges. They cover, from both theoretical and observational perspectives, the lives of massive galaxies from the formation of the first galaxies;

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Dynamics Of Galaxies

Our understanding of galaxies has advanced significantly in recent years. New observations from ground- and space-based telescopes, the;

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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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Dwarf Galaxies (IAU S344)

, with sections dedicated to: Local Group dwarf galaxies; the interstellar medium and star formation in dwarfs; metallicity, massive stars, and;

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

theoreticians working in black hole astrophysics - from stellar-mass black holes to supermassive ones residing at the centre of galaxies - with the aim;

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Become One

like a Man and a Woman some colliding galaxies eventually merge to form a new whole or become one, while other colliding galaxies eventually;

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Quasars, Redshifts and Controversies

related to quasars' redshifts; quasars and galaxies have an origin far different from that assumed in the 'standard' big-bang model of the;

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The Physics and Evolution of Active Galactic Nuclei

galaxies are explained in detail. Both graduate students and researchers will benefit from Netzer's authoritative contributions to this exciting;

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Clusters of Galaxies Physics and Cosmology

of the most important cosmological probes to test the standard cosmological models. Constraints on the Dark Energy equation of state from the;

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Journeys to the Ends of the Universe

Journeys to the Ends of the Universe presents a tour through the universe from the big bang onward. The book explores the limits;

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Journeys to the Ends of the Universe

Journeys to the Ends of the Universe presents a tour through the universe from the big bang onward. The book explores the limits;

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Matter: A Very Short Introduction

that exists. The remaining 95% comes in two mysterious forms: dark matter, and dark energy. Dark matter is necessary to stop the galaxies from;

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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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Invisible Worlds

-edge technology, and see what cant be seen with the naked eye.Its an eye-opening experience: from the smashing of atoms to the;

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Galaxy Formation and Evolution

topics from these disciplines, all of which are needed to understand how galaxies form and evolve, this book is ideal for researchers entering;

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Einde inhoud

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