- Page 3: Boris V.Vasiliev ASTROPHYSICS and a
- Page 7 and 8: 5 The main parameters of star 29 5.
- Page 9 and 10: 8
- Page 11 and 12: theories of stars that are not purs
- Page 13 and 14: But plasma is an electrically polar
- Page 15 and 16: can be described by definite ration
- Page 17 and 18: But even at so high temperatures, a
- Page 19 and 20: 2.2 The energy-preferable state of
- Page 21 and 22: 20
- Page 23 and 24: 3.2 The equilibrium of a nucleus in
- Page 25 and 26: 24
- Page 27 and 28: As a result, the electric force app
- Page 29 and 30: and in accordance with Eq.(4.11), t
- Page 31 and 32: The total kinetic energy of plasma
- Page 33 and 34: we obtain η = 20 = 6.67, (5.24) 3
- Page 35 and 36: 40 N 35 30 10 9 8 7 6 5 4 3 2 1 A/Z
- Page 37 and 38: One can show it easily, that in thi
- Page 39 and 40: 2.10 log (TR/R o T o ) 1.55 1.00 me
- Page 41 and 42: averaged temperature and averaged p
- Page 43 and 44: log R/R o 1.5 1.3 1.1 0.9 measured
- Page 45 and 46: The Table(6.2). The relations of ma
- Page 47 and 48: The Table(6.2)(continuation). N Sta
- Page 49 and 50: The Table(6.2)(continuation). N Sta
- Page 51 and 52: log T/T o 1.0 0.9 0.8 0.7 0.6 measu
- Page 53 and 54: Figure 6.4: The schematic of the st
- Page 55 and 56:
54
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Simultaneously, the torque of a bal
- Page 59 and 60:
At taking into account above obtain
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60
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of periastron rotation of close bin
- Page 65 and 66:
8.3 The angular velocity of the aps
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N -3.0 -2.5 -2.0 -1.5 -1.0 -0.5 0.0
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Figure 9.1: (a) The power spectrum
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Figure 9.2: (a) The measured power
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9.3 The basic elastic oscillation o
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9.5 The spectrum of solar core osci
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star mass spectrum. At first, we ca
- Page 79 and 80:
where ˜ λ C = m ec is the Compto
- Page 81 and 82:
This energy is many orders of magni
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82
- Page 85 and 86:
Figure 11.1: The steady states of s
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It opens a way to estimate the mass
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N 10 9 8 7 6 5 4 3 2 1 0 1.0 1.1 1.
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This makes it possible to estimate
- Page 93 and 94:
to p F ≈ mc, its energy and press
- Page 95 and 96:
94
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approach to the separation of the E
- Page 99 and 100:
is evident as soon as in this proce
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Figure 12.1: The dependence of the
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Figure 12.2: a) The external radius
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104
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It gives a possibility to conclude
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This allows us to explain the obser
- Page 111 and 112:
[14] Landau L.D. and Lifshits E.M.:
- Page 113 and 114:
N Name of star U P M 1 /M ⊙ M 2 /
- Page 115 and 116:
[9] Gemenez A. and Clausen J.V., Fo
- Page 117 and 118:
[30] Hill G. and Holmgern D.E. Stud
- Page 119 and 120:
[52] Semeniuk I. Apsidal motion in
- Page 121:
[75] Andersen J. and Gimenes A. Abs