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Titlebook: Neutron Stars and Their Birth Events; Wolfgang Kundt Book 1990 Kluwer Academic Publishers 1990 Accretion.Population.Supernova.accretion di

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書目名稱Neutron Stars and Their Birth Events
編輯Wolfgang Kundt
視頻videohttp://file.papertrans.cn/665/664685/664685.mp4
叢書名稱Nato Science Series C:
圖書封面Titlebook: Neutron Stars and Their Birth Events;  Wolfgang Kundt Book 1990 Kluwer Academic Publishers 1990 Accretion.Population.Supernova.accretion di
描述This volume is the documentation of the second Course on ‘Neutron Stars, Active Galactic Nuclei and Jets‘, held at Erice in September 1988. This second Course was devoted to our knowledge about neutron-star sources. The poster spoke of: pulsars, accreting X-ray sources and jet englnes, perhaps also UHE pulsars, X- ra~‘ bursters and black-hole candidat.es. Neutron stars have even been proposed as the primary cosmic-ray boosters. Most of theil‘ properties are stil1 controversial, such as their birth mechanism (neutrino versus magnetic piston), internal structure (neutrons, quarks, strange particles), magnetic, thermal and spin histories, wind generation (hydrogen versus pair plasma, radiation versus centrifugal pressure), magnetospheric structure and accretion modes (along field lines versus quasi-Keplerian). The listed controversies have largely survived through the Course and entered into the proceedings. Several lecturers speak of ‘magnetic-field decay‘ in neutron stars, of the ‘recycling‘ of old pulsars, and of ‘a(chǎn)ccretion-induced collapse‘ of white dwarfs as though such processes were textbook knowledge. Terms and abbreviations like RPSR (=recycled pulsar), spinup line, AIC, and
出版日期Book 1990
關(guān)鍵詞Accretion; Population; Supernova; accretion disk; active galactic nuclei; neutron star; relativistic jet; s
版次1
doihttps://doi.org/10.1007/978-94-009-0515-3
isbn_softcover978-94-010-6718-8
isbn_ebook978-94-009-0515-3Series ISSN 1389-2185
issn_series 1389-2185
copyrightKluwer Academic Publishers 1990
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Millisecond Pulsars: A New Population of Gamma Ray Sources?,heir acceleration, and the observed gamma ray emission may be from the same region, or nearby regions of the magnetosphere. Thus, in an indirect way, the pulsed gamma rays are telling us something about the location of the particle accelerator.
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2D Relativistic Pulsar Winds From Rapidly Rotating Neutron Stars,he hot wind equation for the pair plasma and the relativistic Grad-Schlüter-Shafranov (GSS) equation for the magnetic flux function. The structure of the solutions for the hot pair wind equation is discussed. We also show how self-consistent axisymmetric MHD magnetospheres can be constructed by simu
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Book 1990o the proceedings. Several lecturers speak of ‘magnetic-field decay‘ in neutron stars, of the ‘recycling‘ of old pulsars, and of ‘a(chǎn)ccretion-induced collapse‘ of white dwarfs as though such processes were textbook knowledge. Terms and abbreviations like RPSR (=recycled pulsar), spinup line, AIC, and
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