The University of Southampton
University of Southampton Institutional Repository

GATOS: missing molecular gas in the outflow of NGC5728 revealed by JWST

GATOS: missing molecular gas in the outflow of NGC5728 revealed by JWST
GATOS: missing molecular gas in the outflow of NGC5728 revealed by JWST

The ionisation cones of NGC 5728 have a deficit of molecular gas based on millimetre observations of CO (2-1) emission. Although photoionisation from the active nucleus may lead to suppression of this transition, warm molecular gas can still be present. We report the detection of eight mid-infrared rotational H 2 lines throughout the central kiloparsec, including the ionisation cones, using integral field spectroscopic observations with JWST/MIRI MRS. The H 2 line ratios, characteristic of a power-law temperature distribution, indicate that the gas is warmest where it enters the ionisation cone through disk rotation, suggestive of shock excitation. In the nucleus, where the data can be combined with an additional seven ro-vibrational H 2 transitions, we find that moderate velocity (30 km s -1) shocks in dense (10 5 cm -3) gas, irradiated by an external UV field (G 0 = 10 3), do provide a good match to the full set. The warm molecular gas in the ionisation cone that is traced by the H 2 rotational lines has been heated to temperatures > 200 K. Outside of the ionisation cone the molecular gas kinematics are undisturbed. However, within the ionisation cone, the kinematics are substantially perturbed, indicative of a radial flow, but one that is quantitatively different from the ionised lines. We argue that this outflow is in the plane of the disk, implying a short 50 pc acceleration zone up to speeds of about 400 km s -1 followed by an extended deceleration over ~700 pc where it terminates. The deceleration is due to both the radially increasing galaxy mass, and mass-loading as ambient gas in the disk is swept up.

astro-ph.GA, Galaxies: nuclei, Galaxies: individual: NGC 5728, Galaxies: kinematics and dynamics, Galaxies: active, Galaxies: Seyfert
0004-6361
Davies, R.
b3bce148-1213-4c2e-a3bf-a79fe8360f03
Shimizu, T.
e347089c-c6fc-41da-a5e5-36c36aed666f
Pereira-Santaella, M.
273d2fb4-ea55-4bd1-9031-37bf7a2cda75
Alonso-Herrero, A.
ae11bfb3-7ba7-43a3-a071-8fac055b6f62
Audibert, A.
bccc9ed6-8465-4f2d-8471-9ac846d61d41
Bellocchi, E.
e7dfe770-16bb-48af-b6b3-d74949409512
Boorman, P.
da510f67-4d29-4a89-9f7f-8e223c186daf
Campbell, S.
3bd229d2-0d31-451b-9df8-fb290d45d812
Cao, Y.
dcb20516-5d3f-4eb0-b1a1-4b020397f959
Combes, F.
f579a8bb-a74b-41fd-b046-d6084e59ee4a
Delaney, D.
69a66ccd-7fbb-4b1e-b08d-f6b8f53daa2f
Diaz-Santos, T.
3bba8f94-f3b2-494f-acd1-3f16ca1e7f14
Eisenhauer, F.
aeed4378-2137-4e02-8715-fc9c289a92cd
Arredondo, D. Esparza
0972e38e-5c4a-4867-b04d-748fcfa7b420
Feuchtgruber, H.
dbb5f8c0-245d-48b6-beb7-7a075bfdbac6
Schreiber, N.M. Forster
8bc665c3-2905-4908-b4c3-13708a5916da
Fuller, L.
053d2547-ff0b-49df-a328-0bd6ade59ce4
Gandhi, P.
5bc3b5af-42b0-4dd8-8f1f-f74048d4d4a9
Garcia-Bernete, I.
8ec1dc74-5706-41fe-bb4e-06638981842d
Garcia-Burillo, S.
48a403d9-b21b-4e63-8872-8fe043e213a6
Garcia-Lorenzo, B.
6be802fd-62a5-49d3-bbcc-fde0827d1e72
Genzel, R.
1ab9a7e6-02a6-4990-b229-35dff3c05e10
Gillessen, S.
992e4401-a7cb-46b6-b261-fbe57e5bd1d9
Martin, O. Gonzalez
d93ccb03-5f4e-44f9-acc5-68e2018a4019
Haidar, H.
359d2a22-7454-44eb-84bf-75ed7ccc2815
Munoz, L. Hermosa
9e838376-ae5f-416a-b2bf-63e405620346
Hicks, E.K.S.
ded5dc5d-5c31-46b4-80c6-c6f798a22f7f
Hoenig, S.
be0bb8bc-bdac-4442-8edc-f735834f3917
Imanishi, M.
f74c529e-98a7-4367-875f-053e58922144
Izumi, T.
5c2fb272-9563-48a3-b5e9-d0df2f5f269d
Labiano, A.
59c841a1-579a-40e1-a87b-76e643147522
Leist, M.
99b41384-9c01-438f-b1c3-d67ed6a0e062
Levenson, N.A.
57c66b17-cc66-4e9e-8251-19132426cf57
Lopez-Rodriguez, E.
45cde02b-5e26-4030-a88f-7f69099a5481
Lutz, D.
735e6133-6d65-4bd0-ad00-303c6c4757c2
Ott, T.
7b89f519-489a-49df-b0d8-e5f55cb9450a
Packham, C.
344ad7e0-2c15-4b6a-aaf9-80e02d3736d7
Rabien, S.
9110cea5-4251-4034-a544-60ad858007ee
Almeida, C. Ramos
407b9f57-0072-415e-826d-7f711fc5fe65
Ricci, C.
82c8f75d-8215-4054-8b69-4cd30ab2d774
Rigopoulou, D.
0abdde70-e513-47fa-8bf3-595203aa6a6a
Rosario, D.
3e714b97-1e01-4691-813a-e0f7e510d9de
Rouan, D.
da6eeb8e-dcc2-4c2d-95f1-661b15081cf3
Santos, D.J.D.
d66e8f42-120b-4aa5-aa06-fa3100796d54
Shangguan, J.
67b7af5b-2321-47bb-809d-f611ba02af7e
Stalevski, M.
c951d5be-bf04-47e1-83ac-d671e45c6ee5
Sternberg, A.
0a179884-7518-485f-9fab-4b0168c94f75
Sturm, E.
4dee3638-b540-4c0c-8fbf-b1387562733d
Tacconi, L.
a154d333-059f-4563-8bd4-e24a355c9fd9
Martin, M. Villar
35c63fde-f48a-4f7c-acd8-2cec06ffe882
et al.
Davies, R.
b3bce148-1213-4c2e-a3bf-a79fe8360f03
Shimizu, T.
e347089c-c6fc-41da-a5e5-36c36aed666f
Pereira-Santaella, M.
273d2fb4-ea55-4bd1-9031-37bf7a2cda75
Alonso-Herrero, A.
ae11bfb3-7ba7-43a3-a071-8fac055b6f62
Audibert, A.
bccc9ed6-8465-4f2d-8471-9ac846d61d41
Bellocchi, E.
e7dfe770-16bb-48af-b6b3-d74949409512
Boorman, P.
da510f67-4d29-4a89-9f7f-8e223c186daf
Campbell, S.
3bd229d2-0d31-451b-9df8-fb290d45d812
Cao, Y.
dcb20516-5d3f-4eb0-b1a1-4b020397f959
Combes, F.
f579a8bb-a74b-41fd-b046-d6084e59ee4a
Delaney, D.
69a66ccd-7fbb-4b1e-b08d-f6b8f53daa2f
Diaz-Santos, T.
3bba8f94-f3b2-494f-acd1-3f16ca1e7f14
Eisenhauer, F.
aeed4378-2137-4e02-8715-fc9c289a92cd
Arredondo, D. Esparza
0972e38e-5c4a-4867-b04d-748fcfa7b420
Feuchtgruber, H.
dbb5f8c0-245d-48b6-beb7-7a075bfdbac6
Schreiber, N.M. Forster
8bc665c3-2905-4908-b4c3-13708a5916da
Fuller, L.
053d2547-ff0b-49df-a328-0bd6ade59ce4
Gandhi, P.
5bc3b5af-42b0-4dd8-8f1f-f74048d4d4a9
Garcia-Bernete, I.
8ec1dc74-5706-41fe-bb4e-06638981842d
Garcia-Burillo, S.
48a403d9-b21b-4e63-8872-8fe043e213a6
Garcia-Lorenzo, B.
6be802fd-62a5-49d3-bbcc-fde0827d1e72
Genzel, R.
1ab9a7e6-02a6-4990-b229-35dff3c05e10
Gillessen, S.
992e4401-a7cb-46b6-b261-fbe57e5bd1d9
Martin, O. Gonzalez
d93ccb03-5f4e-44f9-acc5-68e2018a4019
Haidar, H.
359d2a22-7454-44eb-84bf-75ed7ccc2815
Munoz, L. Hermosa
9e838376-ae5f-416a-b2bf-63e405620346
Hicks, E.K.S.
ded5dc5d-5c31-46b4-80c6-c6f798a22f7f
Hoenig, S.
be0bb8bc-bdac-4442-8edc-f735834f3917
Imanishi, M.
f74c529e-98a7-4367-875f-053e58922144
Izumi, T.
5c2fb272-9563-48a3-b5e9-d0df2f5f269d
Labiano, A.
59c841a1-579a-40e1-a87b-76e643147522
Leist, M.
99b41384-9c01-438f-b1c3-d67ed6a0e062
Levenson, N.A.
57c66b17-cc66-4e9e-8251-19132426cf57
Lopez-Rodriguez, E.
45cde02b-5e26-4030-a88f-7f69099a5481
Lutz, D.
735e6133-6d65-4bd0-ad00-303c6c4757c2
Ott, T.
7b89f519-489a-49df-b0d8-e5f55cb9450a
Packham, C.
344ad7e0-2c15-4b6a-aaf9-80e02d3736d7
Rabien, S.
9110cea5-4251-4034-a544-60ad858007ee
Almeida, C. Ramos
407b9f57-0072-415e-826d-7f711fc5fe65
Ricci, C.
82c8f75d-8215-4054-8b69-4cd30ab2d774
Rigopoulou, D.
0abdde70-e513-47fa-8bf3-595203aa6a6a
Rosario, D.
3e714b97-1e01-4691-813a-e0f7e510d9de
Rouan, D.
da6eeb8e-dcc2-4c2d-95f1-661b15081cf3
Santos, D.J.D.
d66e8f42-120b-4aa5-aa06-fa3100796d54
Shangguan, J.
67b7af5b-2321-47bb-809d-f611ba02af7e
Stalevski, M.
c951d5be-bf04-47e1-83ac-d671e45c6ee5
Sternberg, A.
0a179884-7518-485f-9fab-4b0168c94f75
Sturm, E.
4dee3638-b540-4c0c-8fbf-b1387562733d
Tacconi, L.
a154d333-059f-4563-8bd4-e24a355c9fd9
Martin, M. Villar
35c63fde-f48a-4f7c-acd8-2cec06ffe882

Davies, R., Shimizu, T. and Pereira-Santaella, M. , et al. (2024) GATOS: missing molecular gas in the outflow of NGC5728 revealed by JWST. Astronomy & Astrophysics, 689, [A263]. (doi:10.1051/0004-6361/202449875).

Record type: Article

Abstract

The ionisation cones of NGC 5728 have a deficit of molecular gas based on millimetre observations of CO (2-1) emission. Although photoionisation from the active nucleus may lead to suppression of this transition, warm molecular gas can still be present. We report the detection of eight mid-infrared rotational H 2 lines throughout the central kiloparsec, including the ionisation cones, using integral field spectroscopic observations with JWST/MIRI MRS. The H 2 line ratios, characteristic of a power-law temperature distribution, indicate that the gas is warmest where it enters the ionisation cone through disk rotation, suggestive of shock excitation. In the nucleus, where the data can be combined with an additional seven ro-vibrational H 2 transitions, we find that moderate velocity (30 km s -1) shocks in dense (10 5 cm -3) gas, irradiated by an external UV field (G 0 = 10 3), do provide a good match to the full set. The warm molecular gas in the ionisation cone that is traced by the H 2 rotational lines has been heated to temperatures > 200 K. Outside of the ionisation cone the molecular gas kinematics are undisturbed. However, within the ionisation cone, the kinematics are substantially perturbed, indicative of a radial flow, but one that is quantitatively different from the ionised lines. We argue that this outflow is in the plane of the disk, implying a short 50 pc acceleration zone up to speeds of about 400 km s -1 followed by an extended deceleration over ~700 pc where it terminates. The deceleration is due to both the radially increasing galaxy mass, and mass-loading as ambient gas in the disk is swept up.

Text
2406.17072v1 - Author's Original
Available under License Creative Commons Attribution.
Download (2MB)
Text
aa49875-24 - Version of Record
Available under License Creative Commons Attribution.
Download (2MB)

More information

Accepted/In Press date: 24 June 2024
e-pub ahead of print date: 20 September 2024
Keywords: astro-ph.GA, Galaxies: nuclei, Galaxies: individual: NGC 5728, Galaxies: kinematics and dynamics, Galaxies: active, Galaxies: Seyfert

Identifiers

Local EPrints ID: 496344
URI: http://eprints.soton.ac.uk/id/eprint/496344
ISSN: 0004-6361
PURE UUID: 2f77a81e-35a3-4c45-83ae-2ce4d86283b5
ORCID for P. Gandhi: ORCID iD orcid.org/0000-0003-3105-2615

Catalogue record

Date deposited: 12 Dec 2024 17:33
Last modified: 13 Dec 2024 02:47

Export record

Altmetrics

Contributors

Author: R. Davies
Author: T. Shimizu
Author: M. Pereira-Santaella
Author: A. Alonso-Herrero
Author: A. Audibert
Author: E. Bellocchi
Author: P. Boorman
Author: S. Campbell
Author: Y. Cao
Author: F. Combes
Author: D. Delaney
Author: T. Diaz-Santos
Author: F. Eisenhauer
Author: D. Esparza Arredondo
Author: H. Feuchtgruber
Author: N.M. Forster Schreiber
Author: L. Fuller
Author: P. Gandhi ORCID iD
Author: I. Garcia-Bernete
Author: S. Garcia-Burillo
Author: B. Garcia-Lorenzo
Author: R. Genzel
Author: S. Gillessen
Author: O. Gonzalez Martin
Author: H. Haidar
Author: L. Hermosa Munoz
Author: E.K.S. Hicks
Author: S. Hoenig
Author: M. Imanishi
Author: T. Izumi
Author: A. Labiano
Author: M. Leist
Author: N.A. Levenson
Author: E. Lopez-Rodriguez
Author: D. Lutz
Author: T. Ott
Author: C. Packham
Author: S. Rabien
Author: C. Ramos Almeida
Author: C. Ricci
Author: D. Rigopoulou
Author: D. Rosario
Author: D. Rouan
Author: D.J.D. Santos
Author: J. Shangguan
Author: M. Stalevski
Author: A. Sternberg
Author: E. Sturm
Author: L. Tacconi
Author: M. Villar Martin
Corporate Author: et al.

Download statistics

Downloads from ePrints over the past year. Other digital versions may also be available to download e.g. from the publisher's website.

View more statistics

Atom RSS 1.0 RSS 2.0

Contact ePrints Soton: eprints@soton.ac.uk

ePrints Soton supports OAI 2.0 with a base URL of http://eprints.soton.ac.uk/cgi/oai2

This repository has been built using EPrints software, developed at the University of Southampton, but available to everyone to use.

We use cookies to ensure that we give you the best experience on our website. If you continue without changing your settings, we will assume that you are happy to receive cookies on the University of Southampton website.

×