The Effect of Outflow Launching Radial Efficiency of Accretion Disk on the Shape of Emission-Line Profiles

This paper presents a preliminary investigation into the influence of radial behavior of disk outflow on the structure and dynamics of the broad line region (BLR) in active galactic nuclei (AGNs), with an emphasis on how the mass ejection rate contributes to shaping the broad emission-line profiles....

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Main Author: Mohammad Hassan Naddaf
Format: Article
Language:English
Published: MDPI AG 2024-12-01
Series:Universe
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Online Access:https://www.mdpi.com/2218-1997/11/1/8
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author Mohammad Hassan Naddaf
author_facet Mohammad Hassan Naddaf
author_sort Mohammad Hassan Naddaf
collection DOAJ
description This paper presents a preliminary investigation into the influence of radial behavior of disk outflow on the structure and dynamics of the broad line region (BLR) in active galactic nuclei (AGNs), with an emphasis on how the mass ejection rate contributes to shaping the broad emission-line profiles. Specifically, we analyze how varying the radial efficiency of mass loss from accretion disks, driven by radiative dust-based mechanisms, contributes to the distribution of material in the BLR. By exploring different radial scenarios of disk mass loss behavior, we uncover connections between outflow radial efficiency and emission line profiles, particularly for lowly ionized lines. Our findings reveal that while the observed shape of broad emission lines is partially influenced by the radial behavior of the disk outflow, it ultimately depends more critically on the physical conditions of the clouds and the specific approach adopted regarding the emissivity for their contribution to the line formation.
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spelling doaj-art-d5d9c939812647d8ae96a5816ff012d92025-01-24T13:51:28ZengMDPI AGUniverse2218-19972024-12-01111810.3390/universe11010008The Effect of Outflow Launching Radial Efficiency of Accretion Disk on the Shape of Emission-Line ProfilesMohammad Hassan Naddaf0Institut d’Astrophysique et de Géophysique, Université de Liège, Allée du Six Août 19c, Sart-Tilman, B-4000 Liège, BelgiumThis paper presents a preliminary investigation into the influence of radial behavior of disk outflow on the structure and dynamics of the broad line region (BLR) in active galactic nuclei (AGNs), with an emphasis on how the mass ejection rate contributes to shaping the broad emission-line profiles. Specifically, we analyze how varying the radial efficiency of mass loss from accretion disks, driven by radiative dust-based mechanisms, contributes to the distribution of material in the BLR. By exploring different radial scenarios of disk mass loss behavior, we uncover connections between outflow radial efficiency and emission line profiles, particularly for lowly ionized lines. Our findings reveal that while the observed shape of broad emission lines is partially influenced by the radial behavior of the disk outflow, it ultimately depends more critically on the physical conditions of the clouds and the specific approach adopted regarding the emissivity for their contribution to the line formation.https://www.mdpi.com/2218-1997/11/1/8broad line regionoutflow rateactive galaxiesradiation pressureemission-line profiles
spellingShingle Mohammad Hassan Naddaf
The Effect of Outflow Launching Radial Efficiency of Accretion Disk on the Shape of Emission-Line Profiles
Universe
broad line region
outflow rate
active galaxies
radiation pressure
emission-line profiles
title The Effect of Outflow Launching Radial Efficiency of Accretion Disk on the Shape of Emission-Line Profiles
title_full The Effect of Outflow Launching Radial Efficiency of Accretion Disk on the Shape of Emission-Line Profiles
title_fullStr The Effect of Outflow Launching Radial Efficiency of Accretion Disk on the Shape of Emission-Line Profiles
title_full_unstemmed The Effect of Outflow Launching Radial Efficiency of Accretion Disk on the Shape of Emission-Line Profiles
title_short The Effect of Outflow Launching Radial Efficiency of Accretion Disk on the Shape of Emission-Line Profiles
title_sort effect of outflow launching radial efficiency of accretion disk on the shape of emission line profiles
topic broad line region
outflow rate
active galaxies
radiation pressure
emission-line profiles
url https://www.mdpi.com/2218-1997/11/1/8
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