Hostname: page-component-745bb68f8f-5r2nc Total loading time: 0 Render date: 2025-01-11T12:55:24.073Z Has data issue: false hasContentIssue false
  • English
  • Français

Identifying the extent of AGN outflows using spatially resolved gas kinematics

Published online by Cambridge University Press:  29 March 2021

Beena Meena Open the ORCID record for Beena Meena [Opens in a new window] ,
D. M. Crenshaw Open the ORCID record for D. M. Crenshaw [Opens in a new window] ,
T. C. Fischer ,
Henrique R. Schmitt ,
M. Revalski  and
G. E. Polack
Beena Meena
Affiliation:
Department of Physics and Astronomy, Georgia State University, Atlanta, GA, USA email: [email protected]
D. M. Crenshaw
Affiliation:
Department of Physics and Astronomy, Georgia State University, Atlanta, GA, USA email: [email protected]
T. C. Fischer
Affiliation:
Space Telescope Science Institute, Baltimore, MD, USA
Henrique R. Schmitt
Affiliation:
Naval Research Laboratory, Washington D.C., DC, United States
M. Revalski
Affiliation:
Space Telescope Science Institute, Baltimore, MD, USA
G. E. Polack
Affiliation:
Department of Physics and Astronomy, Georgia State University, Atlanta, GA, USA email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We present spatially resolved kinematics of ionized gas in the narrow-line region (NLR) and extended narrow-line region (ENLR) in a sample of nearby active galaxies. Utilizing long-slit spectroscopy from Apache Point Observatory (APO)13s ARC 3.5 m Telescope and Hubble Space Telescope (HST) we analyzed the strong λ5007 Å [O III] emission line profiles and mapped the radial velocity distribution of gas at increasing radii from the center. We identified the extents of Active Galactic Nuclei (AGN) driven outflows in our sample and determined the distances at which the observed gas kinematics is being dominated by the rotation of the host galaxy. We also measured the effectiveness of radiative driving of the ionized gas using mass distribution profiles calculated with two-dimensional modeling of surface brightness profiles in our targets. Finally, we compared our kinematic results of the outflow sizes with the maximum distances at which the gas is being radiatively driven to investigate whether these outflows are capable of disrupting or evacuating the star-forming gas at these distances.

Keywords

galaxies: activeAGNNLRkinematicsfeedbackoutflows
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 15 , Symposium S359: Galaxy Evolution and Feedback across Different Environments , March 2019 , pp. 285 - 287
Copyright
© The Author(s), 2021. Published by Cambridge University Press on behalf of International Astronomical Union

References

Barbosa, F. K. B., et al. 2009, MNRAS, 296, 1 Google Scholar
Bentz, M. C., et al. 2009, ApJ, 697, 1 CrossRefGoogle Scholar
Das, V., et al. 2007, ApJ, 656, 2 CrossRefGoogle Scholar
Fischer, T. C., et al. 2013, ApJ, 209, 1 Google Scholar
Fischer, T. C., et al. 2017, ApJ, 834, 30 CrossRefGoogle Scholar
Riffel, R. A., et al. 2008, MNRAS, 385, 3 CrossRefGoogle Scholar
Schinnerer, E., et al. 1999, ApJ, 533, 2 Google Scholar