Introduction to Stellar Astrophysics: Volume 2

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Cambridge University Press, 26 oct 1989 - 264 páginas
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This comprehensive textbook conveys the basic physical ideas and laws used in the study of the outer layers of a star. The stellar atmosphere emits the light which we see. The only layers of a star where we can get direct information about temperature, pressure and composition are in the atmosphere. This complete account first introduces stellar magnitudes, spectra and temperatures. This is followed by a full discussion of radiative transfer in a stellar atmosphere, which leads to descriptions of line formation, the spectrum of hydrogen, and spectral analysis. Finally the structural components that are accessible, such as the convestion zone, chromosphere, corona, and mass outflow are described. The book will interest any student with a knowledge of physics and mathematics who needs to learn about stellar atmospheres.
 

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Índice

II
1
III
3
IV
6
V
9
VI
11
VII
13
VIII
15
X
18
XLIII
91
XLIV
92
XLVI
101
XLVII
105
XLVIII
107
XLIX
114
L
124
LI
125

XII
22
XIII
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XIV
24
XV
26
XVII
27
XVIII
28
XIX
29
XX
39
XXII
41
XXIII
43
XXIV
45
XXV
46
XXVI
49
XXVII
51
XXIX
52
XXX
55
XXXI
60
XXXII
68
XXXIV
72
XXXV
74
XXXVI
79
XXXVIII
81
XXXIX
83
XL
85
XLI
87
XLII
89
LII
136
LIII
140
LIV
143
LV
147
LVI
163
LVII
165
LVIII
167
LIX
173
LX
174
LXI
177
LXII
182
LXIII
183
LXIV
187
LXV
190
LXVII
197
LXVIII
202
LXIX
215
LXX
221
LXXI
226
LXXII
229
LXXIII
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LXXIV
241
LXXV
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LXXVI
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