Bouquet
发表于 2025-3-26 21:04:08
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pericardium
发表于 2025-3-27 01:28:21
Nato Science Series C:http://image.papertrans.cn/n/image/664687.jpg
Herbivorous
发表于 2025-3-27 05:27:16
https://doi.org/10.1007/978-94-011-3536-8Accretion; Supernova; fluid dynamics; galaxies; neutron star; star; star formation; superconductivity
blight
发表于 2025-3-27 11:49:46
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Stable-Angina
发表于 2025-3-27 16:42:47
The Formation of Neutron Stars in The Galaxy accretion-induced collapse of heavy white dwarfs. This article discusses constraints on both scenarios based on observations of supernovae, supernova remnants, binary radio pulsars and radio pulsars in globular clusters.
苦恼
发表于 2025-3-27 19:19:13
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integrated
发表于 2025-3-28 01:14:34
Superfluid Dynamics in Neutron StarsThis lecture reviews some basic points of superfluid dynamics in neutron stars. Recent developments and open problems are pointed out.
deceive
发表于 2025-3-28 04:02:50
Neutron Stars as Cosmic Hadron Physics Laboratories: What Glitches Teach UsOur present theoretical understanding of the crustal neutron superfluid is reviewed, with particular attention to the information concerning its existence and behavior which can be derived from observations of pulsar glitches and postglitch behavior.
TAP
发表于 2025-3-28 08:53:40
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Hamper
发表于 2025-3-28 11:02:20
The Evolution of Neutron Star Magnetic FieldsIn this article we review the arguments for and against the decay of the magnetic fields of neutron stars, in the light of most recent developments. We conclude that the field decay may only occur when the neutron star has been processed in an interacting binary. Some theoretical models for such an evolution are discussed.