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Title: FEEDBACK FROM MASS OUTFLOWS IN NEARBY ACTIVE GALACTIC NUCLEI. II. OUTFLOWS IN THE NARROW-LINE REGION OF NGC 4151

Abstract

We present a detailed study of active galactic nucleus feedback in the narrow-line region (NLR) of the Seyfert 1 galaxy NGC 4151. We illustrate the data and techniques needed to determine the mass outflow rate ( M-dot {sub out}) and kinetic luminosity (L {sub KE}) of the outflowing ionized gas as a function of position in the NLR. We find that M-dot {sub out} peaks at a value of 3.0 M {sub ☉} yr{sup –1} at a distance of 70 pc from the central supermassive black hole (SMBH), which is about 10 times the outflow rate coming from inside 13 pc, and 230 times the mass accretion rate inferred from the bolometric luminosity of NGC 4151. Thus, most of the outflow must arise from in situ acceleration of ambient gas throughout the NLR. L {sub KE} peaks at 90 pc and drops rapidly thereafter, indicating that most of the kinetic energy is deposited within about 100 pc from the SMBH. Both values exceed the M-dot {sub out} and L {sub KE} determined for the UV/X-ray absorber outflows in NGC 4151, indicating the importance of NLR outflows in providing feedback on scales where circumnuclear star formation and bulge growth occur.

Authors:
;  [1];  [2];  [3]
  1. Department of Physics and Astronomy, Georgia State University, 25 Park Place, Suite 605, Atlanta, GA 30303 (United States)
  2. Institute for Astrophysics and Computational Sciences, Department of Physics, The Catholic University of America, Washington, DC 20064 (United States)
  3. Naval Research Laboratory, Washington, DC 20375 (United States)
Publication Date:
OSTI Identifier:
22364467
Resource Type:
Journal Article
Resource Relation:
Journal Name: Astrophysical Journal; Journal Volume: 799; Journal Issue: 1; Other Information: Country of input: International Atomic Energy Agency (IAEA)
Country of Publication:
United States
Language:
English
Subject:
79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; ACCELERATION; BLACK HOLES; BOLOMETERS; FEEDBACK; GALAXY NUCLEI; LUMINOSITY; MASS; SEYFERT GALAXIES; STAR ACCRETION; STAR CLUSTERS; STARS; X RADIATION

Citation Formats

Crenshaw, D. Michael, Fischer, Travis C., Kraemer, Steven B., and Schmitt, Henrique R., E-mail: crenshaw@astro.gsu.edu, E-mail: fischer@astro.gsu.edu, E-mail: steven.b.kraemer@nasa.gov, E-mail: schmitt.henrique@gmail.com. FEEDBACK FROM MASS OUTFLOWS IN NEARBY ACTIVE GALACTIC NUCLEI. II. OUTFLOWS IN THE NARROW-LINE REGION OF NGC 4151. United States: N. p., 2015. Web. doi:10.1088/0004-637X/799/1/83.
Crenshaw, D. Michael, Fischer, Travis C., Kraemer, Steven B., & Schmitt, Henrique R., E-mail: crenshaw@astro.gsu.edu, E-mail: fischer@astro.gsu.edu, E-mail: steven.b.kraemer@nasa.gov, E-mail: schmitt.henrique@gmail.com. FEEDBACK FROM MASS OUTFLOWS IN NEARBY ACTIVE GALACTIC NUCLEI. II. OUTFLOWS IN THE NARROW-LINE REGION OF NGC 4151. United States. doi:10.1088/0004-637X/799/1/83.
Crenshaw, D. Michael, Fischer, Travis C., Kraemer, Steven B., and Schmitt, Henrique R., E-mail: crenshaw@astro.gsu.edu, E-mail: fischer@astro.gsu.edu, E-mail: steven.b.kraemer@nasa.gov, E-mail: schmitt.henrique@gmail.com. 2015. "FEEDBACK FROM MASS OUTFLOWS IN NEARBY ACTIVE GALACTIC NUCLEI. II. OUTFLOWS IN THE NARROW-LINE REGION OF NGC 4151". United States. doi:10.1088/0004-637X/799/1/83.
@article{osti_22364467,
title = {FEEDBACK FROM MASS OUTFLOWS IN NEARBY ACTIVE GALACTIC NUCLEI. II. OUTFLOWS IN THE NARROW-LINE REGION OF NGC 4151},
author = {Crenshaw, D. Michael and Fischer, Travis C. and Kraemer, Steven B. and Schmitt, Henrique R., E-mail: crenshaw@astro.gsu.edu, E-mail: fischer@astro.gsu.edu, E-mail: steven.b.kraemer@nasa.gov, E-mail: schmitt.henrique@gmail.com},
abstractNote = {We present a detailed study of active galactic nucleus feedback in the narrow-line region (NLR) of the Seyfert 1 galaxy NGC 4151. We illustrate the data and techniques needed to determine the mass outflow rate ( M-dot {sub out}) and kinetic luminosity (L {sub KE}) of the outflowing ionized gas as a function of position in the NLR. We find that M-dot {sub out} peaks at a value of 3.0 M {sub ☉} yr{sup –1} at a distance of 70 pc from the central supermassive black hole (SMBH), which is about 10 times the outflow rate coming from inside 13 pc, and 230 times the mass accretion rate inferred from the bolometric luminosity of NGC 4151. Thus, most of the outflow must arise from in situ acceleration of ambient gas throughout the NLR. L {sub KE} peaks at 90 pc and drops rapidly thereafter, indicating that most of the kinetic energy is deposited within about 100 pc from the SMBH. Both values exceed the M-dot {sub out} and L {sub KE} determined for the UV/X-ray absorber outflows in NGC 4151, indicating the importance of NLR outflows in providing feedback on scales where circumnuclear star formation and bulge growth occur.},
doi = {10.1088/0004-637X/799/1/83},
journal = {Astrophysical Journal},
number = 1,
volume = 799,
place = {United States},
year = 2015,
month = 1
}
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