_version_ 1866914459387166720
author Bianchin, Marina
U, Vivian
Song, Yiqing
Lai, Thomas S. -Y.
Remigio, Raymond P.
Barcos-Munoz, Loreto
Diaz-Santos, Tanio
Armus, Lee
Inami, Hanae
Larson, Kirsten L.
Evans, Aaron S.
Boker, Torsten
Kader, Justin A.
Linden, Sean T.
Charmandaris, Vassilis
Malkan, Matthew A.
Rich, Jeff
Bohn, Thomas
Medling, Anne M.
Stierwalt, Sabrina
Mazzarella, Joseph M.
Law, David R.
Privon, George C.
Aalto, Susanne
Appleton, Philip
Brown, Michael J. I.
Buiten, Victorine A.
Finnerty, Luke
Hayward, Christopher C.
Howell, Justin
Iwasawa, Kazushi
Kemper, Francisca
Marshall, Jason
McKinney, Jed
Muller-Sanchez, Francisco
Murphy, Eric J.
van der Werf, Paul P.
Sanders, David B.
Surace, Jason
author_facet Bianchin, Marina
U, Vivian
Song, Yiqing
Lai, Thomas S. -Y.
Remigio, Raymond P.
Barcos-Munoz, Loreto
Diaz-Santos, Tanio
Armus, Lee
Inami, Hanae
Larson, Kirsten L.
Evans, Aaron S.
Boker, Torsten
Kader, Justin A.
Linden, Sean T.
Charmandaris, Vassilis
Malkan, Matthew A.
Rich, Jeff
Bohn, Thomas
Medling, Anne M.
Stierwalt, Sabrina
Mazzarella, Joseph M.
Law, David R.
Privon, George C.
Aalto, Susanne
Appleton, Philip
Brown, Michael J. I.
Buiten, Victorine A.
Finnerty, Luke
Hayward, Christopher C.
Howell, Justin
Iwasawa, Kazushi
Kemper, Francisca
Marshall, Jason
McKinney, Jed
Muller-Sanchez, Francisco
Murphy, Eric J.
van der Werf, Paul P.
Sanders, David B.
Surace, Jason
contents We present new JWST-NIRSpec IFS data for the luminous infrared galaxy NGC7469: a nearby (70.6Mpc) active galaxy with a Sy 1.5 nucleus that drives a highly ionized gas outflow and a prominent nuclear star-forming ring. Using the superb sensitivity and high spatial resolution of the JWST instrument NIRSpec-IFS, we investigate the role of the Seyfert nucleus in the excitation and dynamics of the circumnuclear gas. Our analysis focuses on the [Fe ii], H2, and hydrogen recombination lines that trace the radiation/shocked-excited molecular and ionized ISM around the AGN. We investigate the gas excitation through H2/Brγ and [Fe ii]/Pa\b{eta} emission line ratios and find that photoionization by the AGN dominates within the central 300 pc of the galaxy and together with a small region show ing signatures of shock-heated gas; these shock-heated regions are likely associated with a compact radio jet. In addition, the velocity field and velocity dispersion maps reveal complex gas kinematics. Rotation is the dominant feature, but we also identify non-circular motions consistent with gas inflows as traced by the velocity residuals and the spiral pattern in the Paα velocity dispersion map. The inflow is consistent with the mass outflow rate and two orders of magnitude higher than the AGN accretion rate. The compact nuclear radio jet has enough power to drive the highly ionized outflow. This scenario suggests that the inflow and outflow are in a self-regulating feeding-feedback process, with a contribution from the radio jet helping to drive the outflow.
format Preprint
id arxiv_https___arxiv_org_abs_2308_00209
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle GOALS-JWST: Gas Dynamics and Excitation in NGC7469 revealed by NIRSpec
Bianchin, Marina
U, Vivian
Song, Yiqing
Lai, Thomas S. -Y.
Remigio, Raymond P.
Barcos-Munoz, Loreto
Diaz-Santos, Tanio
Armus, Lee
Inami, Hanae
Larson, Kirsten L.
Evans, Aaron S.
Boker, Torsten
Kader, Justin A.
Linden, Sean T.
Charmandaris, Vassilis
Malkan, Matthew A.
Rich, Jeff
Bohn, Thomas
Medling, Anne M.
Stierwalt, Sabrina
Mazzarella, Joseph M.
Law, David R.
Privon, George C.
Aalto, Susanne
Appleton, Philip
Brown, Michael J. I.
Buiten, Victorine A.
Finnerty, Luke
Hayward, Christopher C.
Howell, Justin
Iwasawa, Kazushi
Kemper, Francisca
Marshall, Jason
McKinney, Jed
Muller-Sanchez, Francisco
Murphy, Eric J.
van der Werf, Paul P.
Sanders, David B.
Surace, Jason
Astrophysics of Galaxies
We present new JWST-NIRSpec IFS data for the luminous infrared galaxy NGC7469: a nearby (70.6Mpc) active galaxy with a Sy 1.5 nucleus that drives a highly ionized gas outflow and a prominent nuclear star-forming ring. Using the superb sensitivity and high spatial resolution of the JWST instrument NIRSpec-IFS, we investigate the role of the Seyfert nucleus in the excitation and dynamics of the circumnuclear gas. Our analysis focuses on the [Fe ii], H2, and hydrogen recombination lines that trace the radiation/shocked-excited molecular and ionized ISM around the AGN. We investigate the gas excitation through H2/Brγ and [Fe ii]/Pa\b{eta} emission line ratios and find that photoionization by the AGN dominates within the central 300 pc of the galaxy and together with a small region show ing signatures of shock-heated gas; these shock-heated regions are likely associated with a compact radio jet. In addition, the velocity field and velocity dispersion maps reveal complex gas kinematics. Rotation is the dominant feature, but we also identify non-circular motions consistent with gas inflows as traced by the velocity residuals and the spiral pattern in the Paα velocity dispersion map. The inflow is consistent with the mass outflow rate and two orders of magnitude higher than the AGN accretion rate. The compact nuclear radio jet has enough power to drive the highly ionized outflow. This scenario suggests that the inflow and outflow are in a self-regulating feeding-feedback process, with a contribution from the radio jet helping to drive the outflow.
title GOALS-JWST: Gas Dynamics and Excitation in NGC7469 revealed by NIRSpec
topic Astrophysics of Galaxies
url https://arxiv.org/abs/2308.00209