Book Description
A comprehensive introduction to the theory underpinning our study of active galactic nuclei and the ways we observe them.
Author : Hagai Netzer
Publisher : Cambridge University Press
Page : 369 pages
File Size : 17,25 MB
Release : 2013-09-16
Category : Science
ISBN : 1107021510
A comprehensive introduction to the theory underpinning our study of active galactic nuclei and the ways we observe them.
Author : Houjun Mo
Publisher : Cambridge University Press
Page : 841 pages
File Size : 37,47 MB
Release : 2010-05-20
Category : Science
ISBN : 0521857937
A coherent introduction for researchers in astronomy, particle physics, and cosmology on the formation and evolution of galaxies.
Author : International Astronomical Union. Colloquium
Publisher : Cambridge University Press
Page : 586 pages
File Size : 37,72 MB
Release : 2004-12-16
Category : Science
ISBN : 9780521849081
This book contains the proceedings of the International Astronomical Union Colloquium no. 195, held in Torino, Italy in 2004. The meeting investigated the formation of galaxies within a full cosmological context, focusing on the outer regions of galaxy clusters. The observed correlation of optical and radio properties of galaxies with their environment indicates that the formation and evolution of galaxies is intimately linked to the formation of large scale structure. With chapters written by leading authorities in the field, this timely volume investigates the role of the environment in determining the properties of galaxies. It describes the distribution of matter and galaxies on the largest scales in the Universe, the processes of cluster and galaxy formation, their role and interplay. This is a valuable collection of review articles for professional astronomers.
Author : Ignacio Ferreras
Publisher : UCL Press
Page : 200 pages
File Size : 26,49 MB
Release : 2019-04-02
Category : Science
ISBN : 1911307614
Galaxies, along with their underlying dark matter halos, constitute the building blocks of structure in the Universe. Of all fundamental forces, gravity is the dominant one that drives the evolution of structures from small density seeds at early times to the galaxies we see today. The interactions among myriads of stars, or dark matter particles, in a gravitating structure produce a system with fascinating connotations to thermodynamics, with some analogies and some fundamental differences. Ignacio Ferreras presents a concise introduction to extragalactic astrophysics, with emphasis on stellar dynamics, and the growth of density fluctuations in an expanding Universe. Additional chapters are devoted to smaller systems (stellar clusters) and larger ones (galaxy clusters). Fundamentals of Galaxy Dynamics, Formation and Evolution is written for advanced undergraduates and beginning postgraduate students, providing a useful tool to get up to speed in a starting research career. Some of the derivations for the most important results are presented in detail to enable students appreciate the beauty of maths as a tool to understand the workings of galaxies. Each chapter includes a set of problems to help the student advance with the material.
Author : Eija Laurikainen
Publisher : Springer
Page : 480 pages
File Size : 47,44 MB
Release : 2015-09-29
Category : Science
ISBN : 3319193783
This book consists of invited reviews on Galactic Bulges written by experts in the field. A central point of the book is that, while in the standard picture of galaxy formation a significant amount of the baryonic mass is expected to reside in classical bulges, the question what is the fraction of galaxies with no classical bulges in the local Universe has remained open. The most spectacular example of a galaxy with no significant classical bulge is the Milky Way. The reviews of this book attempt to clarify the role of the various types of bulges during the mass build-up of galaxies, based on morphology, kinematics and stellar populations and connecting their properties at low and high redshifts. The observed properties are compared with the predictions of the theoretical models, accounting for the many physical processes leading to the central mass concentration and their destruction in galaxies. This book serves as an entry point for PhD students and non-specialists and as a reference work for researchers in the field.
Author : Carol J. Lonsdale Persson
Publisher :
Page : 0 pages
File Size : 43,5 MB
Release : 1987
Category :
ISBN :
Author : Francoise Combes
Publisher : John Wiley & Sons
Page : 324 pages
File Size : 41,12 MB
Release : 2022-08-23
Category : Science
ISBN : 1394163711
All galaxies host a super-massive black hole in their center. These black holes grow their mass in symbiosis with their host galaxy and moderate their star formation. When matter is driven towards the nucleus, an accretion disk is formed to transfer angular momentum and considerable energy is released when the material falls into the black hole: this is the phenomenon of active galactic nuclei (AGN). A nucleus can shine one thousand times more brightly than the entire galaxy with its 200 billion stars. The nuclear activity can take many forms, from very powerful quasars to more ordinary Seyfert galaxies, passing by radio-galaxies, which eject a collimated plasma at ten times the radius of the galaxy. This book examines all of these manifestations and presents a unified view. When two galaxies merge, a binary black hole is formed and the two black holes will spiral inwards and merge, emitting long gravitational waves, which could be detected by the future LISA satellite.
Author : Eric James Murphy
Publisher :
Page : 830 pages
File Size : 24,14 MB
Release : 2018
Category : Discoveries in science
ISBN : 9781583819197
Author : Donald E. Osterbrock
Publisher : University Science Books
Page : 488 pages
File Size : 14,69 MB
Release : 2006
Category : Science
ISBN : 9781891389344
Thoroughly revised and expanded throughout, the new edition is a graduate-level text and reference book on gaseous nebulae, nova and supernova remnants. Much of the new data and new images are from the Hubble Space Telescope with two wholly new chapters being added along with other new features. The previous edition which was tried and tested for thirty years has now been succeeded by a revised, updated, larger edition, which will be valuable to anyone seriously interested in astrophysics.
Author : Grant Heiken
Publisher : CUP Archive
Page : 796 pages
File Size : 30,79 MB
Release : 1991-04-26
Category : Science
ISBN : 9780521334440
The only work to date to collect data gathered during the American and Soviet missions in an accessible and complete reference of current scientific and technical information about the Moon.