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Theory of neutron star magnetospheres

An incomparable reference for astrophysicists studying pulsars and other kinds of neutron stars, "Theory of Neutron Star Magnetospheres" sums up two decades of astrophysical research. It provides in one volume the most important findings to date on this topic, essential to astrophysicists...

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Detalles Bibliográficos
Autor principal: Curtis Michel, F
Lenguaje:eng
Publicado: University of Chicago Press 1990
Materias:
Acceso en línea:http://cds.cern.ch/record/2218201
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author Curtis Michel, F
author_facet Curtis Michel, F
author_sort Curtis Michel, F
collection CERN
description An incomparable reference for astrophysicists studying pulsars and other kinds of neutron stars, "Theory of Neutron Star Magnetospheres" sums up two decades of astrophysical research. It provides in one volume the most important findings to date on this topic, essential to astrophysicists faced with a huge and widely scattered literature. F. Curtis Michel, who was among the first theorists to propose a neutron star model for radio pulsars, analyzes competing models of pulsars, radio emission models, winds and jets from pulsars, pulsating X-ray sources, gamma-ray burst sources, and other neutron-star driven phenomena. Although the book places primary emphasis on theoretical essentials, it also provides a considerable introduction to the observational data and its organization. Michel emphasizes the problems and uncertainties that have arisen in the research as well as the considerable progress that has been made to date.
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spelling cern-22182012021-04-21T19:31:05Zhttp://cds.cern.ch/record/2218201engCurtis Michel, FTheory of neutron star magnetospheresAstrophysics and AstronomyAn incomparable reference for astrophysicists studying pulsars and other kinds of neutron stars, "Theory of Neutron Star Magnetospheres" sums up two decades of astrophysical research. It provides in one volume the most important findings to date on this topic, essential to astrophysicists faced with a huge and widely scattered literature. F. Curtis Michel, who was among the first theorists to propose a neutron star model for radio pulsars, analyzes competing models of pulsars, radio emission models, winds and jets from pulsars, pulsating X-ray sources, gamma-ray burst sources, and other neutron-star driven phenomena. Although the book places primary emphasis on theoretical essentials, it also provides a considerable introduction to the observational data and its organization. Michel emphasizes the problems and uncertainties that have arisen in the research as well as the considerable progress that has been made to date.University of Chicago Pressoai:cds.cern.ch:22182011990
spellingShingle Astrophysics and Astronomy
Curtis Michel, F
Theory of neutron star magnetospheres
title Theory of neutron star magnetospheres
title_full Theory of neutron star magnetospheres
title_fullStr Theory of neutron star magnetospheres
title_full_unstemmed Theory of neutron star magnetospheres
title_short Theory of neutron star magnetospheres
title_sort theory of neutron star magnetospheres
topic Astrophysics and Astronomy
url http://cds.cern.ch/record/2218201
work_keys_str_mv AT curtismichelf theoryofneutronstarmagnetospheres