FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2000269440> ?p ?o ?g. }

• W2000269440 endingPage "110" @default.
• W2000269440 startingPage "97" @default.
• W2000269440 abstract "We present three-dimensional hydrodynamical simulations of gas flows in the vicinity of an active galactic nucleus (AGN) powered by a precessing accretion disk. We consider the effects of the radiation force from such a disk on its environment on a relatively large scale (up to ~10 pc). We implicitly include the precessing disk by forcing the disk radiation field to precess around a symmetry axis with a given period (P) and a tilt angle (Θ). We study the time evolution of the flows irradiated by the disk and investigate basic dependencies of the flow morphology, mass flux, and angular momentum on different combinations of Θ and P. As this is our first attempt to model such three-dimensional gas flows, we consider a simplest form of radiation force, i.e., force due to electron scattering, and neglect the forces due to line and dust scattering/absorption. Furthermore, the gas is assumed to be nearly isothermal. We find that the gas flow settles into a configuration with two components, (1) an equatorial inflow and (2) a bipolar inflow/outflow, with the outflow leaving the system along the poles (the directions of disk normals). However, the flow does not always reach a steady state. We find that the maximum outflow velocity and the kinetic outflow power at the outer boundary can be reduced significantly with increasing Θ. We also find that the mass inflow rate across the inner boundary does not change significantly with increasing Θ. The amount of the density-weighted mean specific angular momentum deposited in the environment by the precessing disk increases as P approaches the gas free-fall time (tff) and then decreases as P becomes much larger than tff. Generally, the characteristics of the flows are closely related to a combination of P and Θ, but not to P and Θ individually. Our models exhibit helical structures in the weakly collimated outflows. Although on different scales, the model reproduces the - or -shaped density morphology of gas outflows, which are often seen in radio observations of AGNs." @default.
• W2000269440 created "2016-06-24" @default.
• W2000269440 creator A5018193989 @default.
• W2000269440 creator A5039717845 @default.
• W2000269440 date "2008-02-10" @default.
• W2000269440 modified "2023-09-27" @default.
• W2000269440 title "Three‐dimensional Simulations of Inflows Irradiated by a Precessing Accretion Disk in Active Galactic Nuclei: Formation of Outflows" @default.
• W2000269440 cites W1523752271 @default.
• W2000269440 cites W1558297478 @default.
• W2000269440 cites W1964458499 @default.
• W2000269440 cites W1967407002 @default.
• W2000269440 cites W1968997566 @default.
• W2000269440 cites W1969002491 @default.
• W2000269440 cites W1970322375 @default.
• W2000269440 cites W1970431563 @default.
• W2000269440 cites W1975347449 @default.
• W2000269440 cites W1976309623 @default.
• W2000269440 cites W1981081082 @default.
• W2000269440 cites W1982067798 @default.
• W2000269440 cites W1986132467 @default.
• W2000269440 cites W1989199175 @default.
• W2000269440 cites W1989204103 @default.
• W2000269440 cites W1990905945 @default.
• W2000269440 cites W1992072403 @default.
• W2000269440 cites W2000246796 @default.
• W2000269440 cites W2001298730 @default.
• W2000269440 cites W2003913435 @default.
• W2000269440 cites W2005370313 @default.
• W2000269440 cites W2007993160 @default.
• W2000269440 cites W2021414755 @default.
• W2000269440 cites W2021627047 @default.
• W2000269440 cites W2022089674 @default.
• W2000269440 cites W2023776546 @default.
• W2000269440 cites W2025087761 @default.
• W2000269440 cites W2027058913 @default.
• W2000269440 cites W2027867125 @default.
• W2000269440 cites W2029227852 @default.
• W2000269440 cites W2034343521 @default.
• W2000269440 cites W2035478725 @default.
• W2000269440 cites W2036257139 @default.
• W2000269440 cites W2039518933 @default.
• W2000269440 cites W2039714125 @default.
• W2000269440 cites W2040723374 @default.
• W2000269440 cites W2042259048 @default.
• W2000269440 cites W2046321578 @default.
• W2000269440 cites W2057023417 @default.
• W2000269440 cites W2061435934 @default.
• W2000269440 cites W2062393186 @default.
• W2000269440 cites W2065116379 @default.
• W2000269440 cites W2065580778 @default.
• W2000269440 cites W2065924775 @default.
• W2000269440 cites W2066744800 @default.
• W2000269440 cites W2066886457 @default.
• W2000269440 cites W2067366609 @default.
• W2000269440 cites W2071675272 @default.
• W2000269440 cites W2072637512 @default.
• W2000269440 cites W2072698226 @default.
• W2000269440 cites W2074119073 @default.
• W2000269440 cites W2079040992 @default.
• W2000269440 cites W2082225226 @default.
• W2000269440 cites W2082636340 @default.
• W2000269440 cites W2083607162 @default.
• W2000269440 cites W2093419164 @default.
• W2000269440 cites W2093609791 @default.
• W2000269440 cites W2094935422 @default.
• W2000269440 cites W2095427738 @default.
• W2000269440 cites W2109074901 @default.
• W2000269440 cites W2113491874 @default.
• W2000269440 cites W2123036634 @default.
• W2000269440 cites W2126019686 @default.
• W2000269440 cites W2131276846 @default.
• W2000269440 cites W2133778146 @default.
• W2000269440 cites W2134866927 @default.
• W2000269440 cites W2139412687 @default.
• W2000269440 cites W2154955582 @default.
• W2000269440 cites W2156621121 @default.
• W2000269440 cites W2162132003 @default.
• W2000269440 cites W2162195514 @default.
• W2000269440 cites W2165911809 @default.
• W2000269440 cites W3013051201 @default.
• W2000269440 cites W3013241125 @default.
• W2000269440 cites W3098312899 @default.
• W2000269440 cites W3098900999 @default.
• W2000269440 cites W3099354128 @default.
• W2000269440 cites W3100098924 @default.
• W2000269440 cites W3100782618 @default.
• W2000269440 cites W3102053561 @default.
• W2000269440 cites W3102216133 @default.
• W2000269440 cites W3103097416 @default.
• W2000269440 cites W3103139228 @default.
• W2000269440 cites W3104428752 @default.
• W2000269440 cites W3104827874 @default.
• W2000269440 cites W3105291241 @default.
• W2000269440 cites W3106157876 @default.
• W2000269440 cites W3106239262 @default.
• W2000269440 cites W3122565141 @default.
• W2000269440 cites W4299527096 @default.
• W2000269440 cites W2083972563 @default.

• next