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Titlebook: Neutron Stars and Pulsars; Werner Becker Book 2009 Springer-Verlag Berlin Heidelberg 2009 Gravitational Waves from Spinning Neutron Stars.

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發(fā)表于 2025-3-26 21:42:52 | 只看該作者
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發(fā)表于 2025-3-27 02:34:20 | 只看該作者
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發(fā)表于 2025-3-27 07:06:50 | 只看該作者
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發(fā)表于 2025-3-27 12:22:07 | 只看該作者
The Theory of Pulsar Winds and Nebulae, already apparent that the magnetic field and relativistic particles that produce the radiation of the Crab Nebula must have their origin in a central stellar object [104]. Today, about 50 similarly powered objects are known, and some of them, like the Crab, are detected and even resolved at all acc
35#
發(fā)表于 2025-3-27 15:29:43 | 只看該作者
Implications of HESS Observations of Pulsar,ith rela-tivistic electrons moving in magnetized plasmas to give the continuum radiation as observed. Visionaries like [36] already predicted that we should be able to measure the magnetic field strength in PWN using the combination of synchrotron and inverse Compton (IC) radiation. Following this,
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發(fā)表于 2025-3-27 20:42:34 | 只看該作者
37#
發(fā)表于 2025-3-28 00:11:16 | 只看該作者
High-energy Emission from the Polar Cap and Slot Gap,here have been some fundamental developments in acceleration and emission models. In this Chapter I will review both the basic physics of the models as well as the latest developments in understanding the high-energy emission of rotation-powered pulsars, with particular emphasis on the polar-cap and
38#
發(fā)表于 2025-3-28 04:11:23 | 只看該作者
39#
發(fā)表于 2025-3-28 09:12:28 | 只看該作者
https://doi.org/10.1007/978-3-540-76965-1Gravitational Waves from Spinning Neutron Stars; Gravity; Isolated Neutron Stars and Millisecond Pulsa
40#
發(fā)表于 2025-3-28 11:32:15 | 只看該作者
Werner BeckerComprehensive reference written by leading international experts.Reviews historical development in pulsar research and presents current understanding and open questions.Includes supplementary material
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