TY - BOOK ID - 113574245 TI - Global Understanding of Accretion and Ejection around Black Holes PY - 2022 SN - 3036556095 3036556109 PB - Basel MDPI - Multidisciplinary Digital Publishing Institute DB - UniCat KW - Research & information: general KW - Physics KW - Astronomy, space & time KW - black hole physics KW - rotating black holes KW - relativistic jets KW - active galactic nuclei KW - supermassive black holes KW - radio galaxies KW - galaxies: active KW - galaxies: jets KW - galaxies: nuclei KW - radiative transfer KW - Seyfert 1 objects: individual: Mrk 335 KW - X-Rays:binaries—stars individual: (XTE J1908+094)—stars:black holes—accretion KW - accretion disks—shock waves—radiation:dynamics KW - X-rays: binaries—stars individual: (V404 Cygni)—stars:black holes—accretion KW - isofrequency KW - geodesic orbits KW - black string KW - black hole evolution KW - supermassive black hole KW - accretion of matter KW - galaxies: evolution KW - galaxies KW - active KW - galaxies–quasars KW - individual (Ton 599) KW - BL lacertae objects KW - OJ 287 KW - accretion discs KW - gravitational waves KW - jets KW - blazars KW - X-rays KW - synchrotron emission KW - inverse-Compton emission KW - optical spectroscopy KW - ionized gas KW - broad line region KW - n/a KW - X-Rays:binaries-stars individual: (XTE J1908+094)-stars:black holes-accretion KW - accretion disks-shock waves-radiation:dynamics KW - X-rays: binaries-stars individual: (V404 Cygni)-stars:black holes-accretion KW - galaxies-quasars UR - https://www.unicat.be/uniCat?func=search&query=sysid:113574245 AB - Accretion-ejection around compact objects, mainly around black holes, both in low mass, supermassive, and intermediate-mass, are rich and has been studied exhaustively. However, the subject is expanding and growing rapidly after the launch of different space-based satellites and ground-based telescopes in multiwavelength bands, leaving a range of questions on accretion and ejection mechanisms. The proper understanding of the underlying physical mechanisms responsible for observational evidence is still lacking for several reasons. With the advent of high-resolution satellite observations, it is possible to look at the problems globally as a complete package in a more consistent way. Recently, many new low mass black hole candidates have been discovered; however, very little is known about those systems, e.g., mass, spin parameter, and orbital period. The study in the spectro-temporal domain also needs proper understanding of spectral state change, quasi-periodic oscillation frequency evolution, hardness intensity diagram, and line emissions. The goal and motivation of this book are to focus on top-quality original works in the above-mentioned context, with important research facts that are written in a highly understandable way, from a theoretical, observational, and numerical simulation ground.This book is a collection of high-quality research work, which will give a compact and concise description of the overall view of the subject. ER -