Science bin
Accretion disks
Accretion Flows in Astrophysics (Ed. N. I. Shakura) 2018, DOI
https://doi.org/10.1007/978-3-319-93009-1
1st chapter by G. Lipunova, K. Malanchev, and N. Shakura
bookmetrix
Аккреционные диски. Стандартная модель. - исправленная версия (июль
2023) -
1 Глава из книги под общей редакцией Шакуры Н.И., авторы главы: Липунова Г.В., Маланчев К.Л.; ( версия марта 2016 г. ). См также всю книгу
Аккреционные процессы в астрофизике. Физматлит 2015, авторы
Аболмасов П.К., Постнов К.А., Журавлев В.В., Кочеткова А.Ю., Липунова Г.В., Маланчев К.Л., Раздобурдин Д.Н., Чашкина А.А., Шакура Н.И., Ялмарсдоттер В.
под общей редакцией Н.И.Шакуры
Freddi : the code
/ http://ascl.net/1610.014
by K. Malanchev to compute FRED-like light curves of LMXB calculate evolution of the
accretion disk with time-independent viscosity in a binary system
The code solves 1-D evolution equation of Shakura-Sunyaev accretion disk. The code is developed to simulate fast rise exponential decay (FRED) light curves of low mass X-ray binaries (LMXBs) and is briefly described in “Determination of the turbulent parameter in the accretion disks: effects of self-irradiation in 4U 1543-47 during the 2002 outburst” by Lipunova & Malanchev
(2016)
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
-
plot
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 ).
Dimensionless Pi values from the solution of the vertical structure of standard accretion disc, zone B and C Ketsaris and Shakura (1998) . See paragraph 1.5
Tidal radius illustration following works by
Paczynski (1977, P77) ;
Papaloizou & Pringle (1977, PP77) ;
Gilfanov & Arefiev (2005, GA2005)
Список литературы и ссылок по темам Аккреция, диски, рентгеновские транзиенты...
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Data
Outbursts
A 0620-00 (1975) and GS 1124-68 (1991)
AMXP outbursts
Optical filters (coming...)
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MASTER
Наблюдения с поляроидами в системе МАСТЕР c двумя трубами
MEMO October 2013
MASTER Absolute Photometric Calibration
for observations with polarizers
Analysis of linear polarization basing on the single Stokes parameter
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Семинары
В отделе релятивистской астрофизики ГАИШ МГУ
Общемосковский семинар астрофизиков им. Я.Б.Зельдовича (ОСА)
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Reading / Tools
Accretion Disks by Н. С. Spruit
Essential magnetohydrodynamics for astrophysics by Н. С. Spruit
Various reviews
Список литературы и ссылок по темам Аккреция, диски, рентгеновские транзиенты...
Help on Maple (Peter Stone's Maple Worksheets)
Maple Advisor Database
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