dejected 发表于 2025-3-21 17:56:43
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Neutron Stars 1978-0-387-47301-7Series ISSN 0067-0057 Series E-ISSN 2214-7985discord 发表于 2025-3-22 01:19:01
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Astrophysics and Space Science Libraryhttp://image.papertrans.cn/n/image/664683.jpgMITE 发表于 2025-3-22 19:53:11
https://doi.org/10.1007/978-0-387-47301-7Star; Universe; book about neutron stars; dense matter; neutron star composition; neutron star magnetic f大范围流行 发表于 2025-3-22 23:14:21
Overview, ∼ 1.4M⊙ and radii R ∼ 10 km. Thus, their masses are close to the solar mass M⊙ = 1.989 × 10. g, but their radii are ∼ 10. times smaller than the solar radius R⊙ = 6.96×10. km. Accordingly, neutron stars possess an enormous gravitational energy . and surface gravity ., . where . is the gravitational忍耐 发表于 2025-3-23 01:25:21
Equilibrium Plasma Properties. Outer Envelopes,oted to neutron star envelopes. These envelopes are non-uniform. The structure of an envelope for a star with the effective surface temperature ∼ 10. K is schematically shown in Fig. 2.1. We indicate characteristic densities and geometrical depths of interfaces between adjoining layers. One can distarrhythmic 发表于 2025-3-23 08:50:14
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