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оригинального документа
: http://xray.sai.msu.ru/~galja/resources.html
Дата изменения: Thu Mar 31 11:39:51 2016
Дата индексирования: Sat Apr 9 23:03:38 2016
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Поисковые слова: jupiter
C-code to calculate evolution of the
accretion disk with time-independent viscosity in a binary system (v0.3 March 2015)
(
см. ApJ 2015 ).
Multi-color black body disk dimensionless spectrum for values: Fnu/Fmax
vs. x = h nu/ kTmax, where Tmax - maximum temperature of Shakura-Sunyaev disk
table
-
иллюстрация
Angular dependence Psi(theta) of intensity from accretion disk in Kerr-metric.
Observed flux F=L*Psi(theta)/(4 pi D)^2, where L is the bolometric luminosity,
D is the distance to the disk, theta is the angle between the normal to the
disk plane and the line of sight, mu = cos(theta), mu=0 when photons go
parallel to the disk plane.
a=0.0
;
a=0.9981
;
Functions are calculated using different codes: kerrbb
(Li et al., 2005),
Laor-Netzer
(1990), and
Speith et al.
(1995). Cumulative "INT"-curves are integrated over the angle.
(
см. AЖ 2007 ).