ESCAPE OF RESONANCE-LINE RADIATION FROM AN OPTICALLY THICK NEBULA

被引:196
作者
OSTERBROCK, DE
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10.1086/147258
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P1 [天文学];
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0704 ;
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页码:195 / &
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共 33 条
[1]  
Ambarzumian V.A., 1958, THEORETICAL ASTROPHY
[2]   The radiative equilibrium of a planetary nebula [J].
Ambarzumian, VA .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1932, 93 (01) :0050-0061
[3]   Physical processes in gaseous nebulae III. The Balmer decrement [J].
Baker, JG ;
Menzel, DH .
ASTROPHYSICAL JOURNAL, 1938, 88 (01) :52-64
[4]  
Bethe H., 1933, HDB PHYS, V24, P273
[5]   Stochastic problems in physics and astronomy [J].
Chandrasekhar, S .
REVIEWS OF MODERN PHYSICS, 1943, 15 (01) :0001-0089
[6]   THE TIME RELAXATION OF A RESONANCE-LINE PROFILE [J].
FIELD, GB .
ASTROPHYSICAL JOURNAL, 1959, 129 (03) :551-564
[7]  
GREEN LC, 1957, ASTROPHYS J S, V3, P37
[8]   ON THE LINE-ABSORPTION COEFFICIENT DUE TO DOPPLER EFFECT AND DAMPING [J].
HARRIS, DL .
ASTROPHYSICAL JOURNAL, 1948, 108 (01) :112-115
[9]  
HENYEY LG, 1940, ASTROPHYS J, V26, P50
[10]  
JAGER CD, 1959, HDB PHYS, V51, P80