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This book reviews the phenomenology displayed by relativistic jets
as well as the most recent theoretical efforts to understand the
physical mechanisms at their origin. Relativistic jets have been
observed and studied in Active Galactic Nuclei (AGN) for about half
a century and are believed to be fueled by accretion onto a
supermassive black hole at the center of the host galaxy. Since the
first discovery of relativistic jets associated with so-called
"micro-quasars" much more recently, it has seemed clear that much
of the physics governing the relativistic outflows in stellar X-ray
binaries harboring black holes and in AGN must be common, but
acting on very different spatial and temporal scales. With new
observational and theoretical results piling up every day, this
book attempts to synthesize a consistent, unified physical picture
of the formation and disruption of jets in accreting black-hole
systems. The chapters in this book offer overviews accessible not
only to specialists but also to graduate students and
astrophysicists working in other areas. Covered topics comprise
Relativistic jets in stellar systems Launching of AGN jets
Parsec-scale AGN jets Kiloparsec-scale AGN jets Black hole
magnetospheres Theory of relativistic jets The structure and
dynamics of the inner accretion disk The origin of the jet magnetic
field X-ray observations, phenomenology, and connection with theory
This book reviews the phenomenology displayed by relativistic jets
as well as the most recent theoretical efforts to understand the
physical mechanisms at their origin. Relativistic jets have been
observed and studied in Active Galactic Nuclei (AGN) for about half
a century and are believed to be fueled by accretion onto a
supermassive black hole at the center of the host galaxy. Since the
first discovery of relativistic jets associated with so-called
"micro-quasars" much more recently, it has seemed clear that much
of the physics governing the relativistic outflows in stellar X-ray
binaries harboring black holes and in AGN must be common, but
acting on very different spatial and temporal scales. With new
observational and theoretical results piling up every day, this
book attempts to synthesize a consistent, unified physical picture
of the formation and disruption of jets in accreting black-hole
systems. The chapters in this book offer overviews accessible not
only to specialists but also to graduate students and
astrophysicists working in other areas. Covered topics comprise
Relativistic jets in stellar systems Launching of AGN jets
Parsec-scale AGN jets Kiloparsec-scale AGN jets Black hole
magnetospheres Theory of relativistic jets The structure and
dynamics of the inner accretion disk The origin of the jet magnetic
field X-ray observations, phenomenology, and connection with theory
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