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Titlebook: Cosmical Magnetism; D. Lynden-Bell Book 1994 Springer Science+Business Media Dordrecht 1994 Scale.astronomy.magnetosphere.quasar.relativis

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书目名称Cosmical Magnetism
编辑D. Lynden-Bell
视频videohttp://file.papertrans.cn/239/238904/238904.mp4
丛书名称Nato Science Series C:
图书封面Titlebook: Cosmical Magnetism;  D. Lynden-Bell Book 1994 Springer Science+Business Media Dordrecht 1994 Scale.astronomy.magnetosphere.quasar.relativis
描述Prof. Leon Mestel has been an inspiration to many to study the role of magnetism in the Cosmos. To mark the occasion of his retin‘ment from the University of Sussex after 43 years in astrophysics, several of his friends and former students decided to hold an advanced research workshop in his honour. NATO agreed to finance this venture which was held at the Institute of Astronomy at Cambridge. The scientific organizing committee was J. Landstreet, D. Lynden-Bell, F. Pacini, M.A. Rud0rman and N.O. Weiss and most leading experts on Cosmical magnetism agreed to come. We are particularly grateful to Lyman Spitzer who, ably helped by his wife Doreen, !!;ave the after dinner addre~s on how the goddess Astrophysica had foreseen Leon‘s achievements in classical Greek times. Not without regret we decided to maintain the homog0neity of the material and therefore could not cover Leon Mestel‘s major achievements in non-magnetic astronomy. His work on the cooling of white dwarfs, his understanding that degenerate hydrogen was a nuclear explosive since its pressure was almost independent of temperature and hence, his picture of supernovae, which is now more commonly applied to novae, his seminal
出版日期Book 1994
关键词Scale; astronomy; magnetosphere; quasar; relativistic jet
版次1
doihttps://doi.org/10.1007/978-94-011-1110-2
isbn_softcover978-94-010-4485-1
isbn_ebook978-94-011-1110-2Series ISSN 1389-2185
issn_series 1389-2185
copyrightSpringer Science+Business Media Dordrecht 1994
The information of publication is updating

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Introduction: The Written Constitution,equences include the formation of weak dipole moment millisecond pulsars by the accretion induced spin-up of strong field neutron stars, the absence of observable spin modulation of the thermal X-ray emission from the surfaces of neutron stars in accreting low mass X-ray binaries (LMXB’s), pulsar pe
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