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@article{2239829,
author = {Naddaf, MohammadandHassan and Czerny, Bozena and Zajaček, Michal},
article_number = {3},
doi = {http://dx.doi.org/10.3390/dynamics2030015},
keywords = {super-Eddington accretion disk; active galaxies; broad-line region; dust-driving mechanism; radiation pressure; FRADO model},
language = {eng},
issn = {2673-8716},
journal = {Dynamics},
title = {The Wind Dynamics of Super-Eddington Sources in FRADO},
url = {https://www.mdpi.com/2673-8716/2/3/15},
volume = {2},
year = {2022}
}
TY - JOUR
ID - 2239829
AU - Naddaf, Mohammad-Hassan - Czerny, Bozena - Zajaček, Michal
PY - 2022
TI - The Wind Dynamics of Super-Eddington Sources in FRADO
JF - Dynamics
VL - 2
IS - 3
SP - 295-305
EP - 295-305
PB - MDPI
SN - 26738716
KW - super-Eddington accretion disk
KW - active galaxies
KW - broad-line region
KW - dust-driving mechanism
KW - radiation pressure
KW - FRADO model
UR - https://www.mdpi.com/2673-8716/2/3/15
N2 - We perform non-hydrodynamical 2.5D simulations to study the dynamics of material above accretion disk based on the disk radiation pressure acting on dust. We assume a super-accreting underlying disk with the accretion rate of 10 times the Eddington rate with central black hole mass ranging from 107 up to 109M⊙. Such high accretion rates are characteristic for extreme sources. We show that for high accretors the radiatively dust-driving mechanism based on the FRADO model always leads to a massive outflow from the disk surface, and the failed wind develops only at larger radii. The outflow rate strongly depends on the black hole mass, and an optically thick energy-driven solution can exceed the accretion rate for masses larger than 108M⊙ but momentum-driven outflow does not exceed the accretion rate even for super-Eddington accretion, therefore not violating the adopted stationarity of the disk. However, even in this case the outflow from the disk implies a strong mechanical feedback.
ER -
NADDAF, Mohammad-Hassan, Bozena CZERNY a Michal ZAJAČEK. The Wind Dynamics of Super-Eddington Sources in FRADO. \textit{Dynamics}. MDPI, 2022, roč.~2, č.~3, s.~295-305. ISSN~2673-8716. Dostupné z: https://dx.doi.org/10.3390/dynamics2030015.
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