2026A&A...705A.249O


Query : 2026A&A...705A.249O

2026A&A...705A.249O - Astronomy and Astrophysics, volume 705A249 (2026/1-1)

The relationship between warm and hot gas-phase metallicity in massive elliptical galaxies and the influence of active galactic nucleus feedback.

OLIVARES V., SU Y., TEMI P., ESKENASY R., RUSSELL H., GASPARI M., SALOME P., COMBES F., SUN M., TREISTER E., FOGARTY K., JIMENEZ-GALLARDO A. and LAGOS P.

Abstract (from CDS):

Context. Warm ionized gas is ubiquitous at the centers of X-ray bright elliptical galaxies. While it is believed to play a key role in the feeding and feedback processes of supermassive black holes, its origins remain under debate. Existing studies have primarily focused on the morphology and kinematics of warm ionized gas.
Aims. This work aims to provide a new perspective on warm (∼10 000 K) ionized gas and its connection to X-ray-emitting hot gas (> 106 K) by measuring and comparing their metallicities.
Methods. We conducted a joint analysis of 13 massive elliptical galaxies using MUSE/VLT and Chandra observations. Emission-line ratios, including [OIII]/Hβ, [NII]/Hα, were measured using MUSE observations to infer the ionization mechanisms. We derive metallicities of the warm ionized gas using HII, and LINER calibrations. We also computed the warm phase metallicity using X-ray/EUV, and pAGB star models. For two sources at higher redshifts, the direct Te method was also used to measure warm gas metallicities. The metallicity of the hot gas was measured using Chandra X-ray observations.
Results. Our observations reveal that most sources exhibit composite ionization, with contributions from both star formation and LINER-like emission. The four sources with the lowest star formation rates in our sample - Centaurus, M87, M84, and Abell 496 - are dominated by LINER emission. A positive linear correlation was found between the gas-phase metallicities of the warm and hot phases, ranging from 0.3 to 1.5 Z⊙. In some sources the warm gas metallicity shows a central drop. A similar radial trend has been reported for the hot gas metallicity in some galaxy clusters.
Conclusions. The ionization mechanisms of cooling flow elliptical galaxies are diverse, suggesting multiple channels for powering the warm ionized gas. The positive correlation found in warm and hot gas metallicities suggest the intimate connection between the two gas phases, likely driven by gas cooling and/or mixing. The large variation in the warm gas metallicity further suggests that cold gas mass derived under the assumption of solar metallicity for the CO-to-H2 conversion factor needs to be revised by approximately an order of magnitude.

Abstract Copyright: © The Authors 2026

Journal keyword(s): ISM: abundances - galaxies: abundances - galaxies: clusters: general - galaxies: clusters: intracluster medium

Simbad objects: 14

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Number of rows : 14
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 ZwCl 0335+0956 ClG 03 38 35.3 +09 57 54           ~ 402 1
2 ACO 496 ClG 04 33 40.8 -13 14 34           ~ 728 2
3 PKS 0745-19 rG 07 47 31.3247085936 -19 17 40.013334276   19.60       ~ 422 1
4 BAX 125.2599+07.8631 ClG 08 21 02.4 +07 51 47           ~ 72 1
5 MCG-02-24-007 LIN 09 18 05.66848602 -12 05 43.8060823   14.38 14.8     ~ 1077 1
6 M 84 Sy2 12 25 03.74333 +12 53 13.1393 12.67 12.09 10.49     ~ 1841 2
7 M 87 AGN 12 30 49.42338414 +12 23 28.0436859 10.16 9.59 8.63   7.49 ~ 7815 3
8 NGC 4696 rG 12 48 49.2724775784 -41 18 39.304053252   11.21   10.7   ~ 510 3
9 ACO 1795 ClG 13 48 47.4 +26 34 55           ~ 1330 0
10 ACO 1835 ClG 14 01 02.07 +02 52 43.2           ~ 727 1
11 NGC 5846 rG 15 06 29.253 +01 36 20.29   11.9   9.74   ~ 891 2
12 ClG J1931-2635 ClG 19 31 49.6 -26 34 33           ~ 181 0
13 ACO S 1101 ClG 23 13 58.5 -42 43 39           ~ 272 1
14 ACO 2597 ClG 23 25 19.70 -12 07 27.7           ~ 572 0

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