恒星结构与演化-第二版-(影印版) 本书特色

《恒星结构与演化（第二版）(英文影印版)》详细地介绍了恒星的结构和演化理论。从恒星的组成成分讲起，讲解了恒星中的热核反应过程、热核反应之后的产物、超新星爆发等等一系列想象和理论。对于白矮星、中子星和黑洞也都做了详细介绍。本书适合天体物理方向的科研工作者和研究生阅读。

恒星结构与演化-第二版-(影印版) 内容简介

恒星是*常见的星体。满天星斗中，除了有限的几颗外都是恒星。而白矮星、中子星和黑洞也都是恒星演化的产物。恒星并不能恒久存在，也有初生、也会死亡。《恒星结构与演化（第二版）(英文影印版)》正是刻画恒星壮丽一生的学术著作。科研工作者乃至有一定基础的天文爱好者都不应错过这一佳作。

恒星结构与演化-第二版-(影印版) 目录

part i the basic equations

1 coordinates, mass distribution, and gravitational field
in spherical stars
1.1 eulerian description
1.2 lagrangian description
1.3 the gravitational field

2 conservation of momentum
2.1 hydrostatic equilibrium
2.2 the role of density and simple solutions
2.3 simple estimates of central values pc; tc
2.4 the equation of motion for spherical symmetry
2.5 the non-spherical case
2.6 hydrostatic equilibrium in general relativity
2.7 the piston model

3 the virial theorem
3.1 stars in hydrostatic equilibrium
3.2 the virial theorem of the piston model
3.3 the kelvin-helmholtz timescale
3.4 the virial theorem for non-vanishing surface pressure

4 conservation of energy
4.1 thermodynamic relations
4.2 the perfect gas and the mean molecularweight
4.3 thermodynamic quantities for the perfect, monatomic gas
4.4 energy conservation in stars
4.5 global and local energy conservation
4.6 timescales

5 transport of energy by radiation and conduction
5.1 radiative transport of energy
5.1.1 basic estimates
5.1.2 diffusion of radiative energy
5.1.3 the rosseland mean for
5.2 conductive transport of energy
5.3 the thermal adjustment time of a star
5.4 thermal properties of the piston model

6 stability against local, non-spherical perturbations
6.1 dynamical instability
6.2 oscillation of a displaced element
6.3 vibrational stability
6.4 the thermal adjustment time
6.5 secular instability
6.6 the stability of the piston model

7 transport of energy by convection
7.1 the basic picture
7.2 dimensionless equations
7.3 limiting cases, solutions, discussion
7.4 extensions of the mixing-length theory

8 the chemical composition
8.1 relative mass abundances
8.2 variation of composition with time
8.2.1 radiative regions
8.2.2 diffusion
8.2.3 convective regions

9 mass loss

part ii the overall problem

10 the differential equations of stellar evolution
10.1 the full set of equations
10.2 timescales and simplifications

11 boundary conditions
11.1 central conditions
11.2 surface conditions
11.3 influence of the surface conditions and properties of
envelope solutions
11.3.1 radiative envelopes
11.3.2 convective envelopes
11.3.3 summary
11.3.4 the t _r stratification

12 numerical procedure
12.1 the shootingmethod
12.2 the henyey method
12.3 treatment of the first- and second-order time derivatives
12.4 treatment of the diffusion equation
12.5 treatment of mass loss
12.6 existence and uniqueness

part iii properties of stellar matter

13 the perfect gas with radiation
13.1 radiation pressure
13.2 thermodynamic quantities

14 ionization
14.1 the boltzmann and saha formulae
14.2 ionization of hydrogen
14.3 thermodynamical quantities for a pure hydrogen gas
14.4 hydrogen-heliummixture
14.5 the general case
14.6 limitation of the saha formula

15 the degenerate electron gas
15.1 consequences of the pauli principle
15.2 the completely degenerate electron gas

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自然科学 天文学

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