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Complex Velocity Structure of Nebular Gas in Active Galaxies Centred in Cooling X-ray Atmospheres

Gingras, Marie-Joëlle; Coil, Alison L; Mcnamara, B R; Perrotta, Serena; Brighenti, Fabrizio; Russell, H R; Li, Muzi; Peng Oh, S; Wenmeng, Wenmeng

Complex Velocity Structure of Nebular Gas in Active Galaxies Centred in Cooling X-ray Atmospheres Thumbnail


Authors

Marie-Joëlle Gingras

Alison L Coil

B R Mcnamara

Serena Perrotta

Fabrizio Brighenti

Muzi Li

S Peng Oh

Wenmeng Wenmeng



Abstract

[OII] emission maps obtained with the Keck Cosmic Web Imager (KCWI) are presented for four galaxies centered in cooling X-ray cluster atmospheres. Nebular emission extending tens of kpc is found in systems covering a broad range of atmospheric cooling rates, cluster masses, and dynamical states. Abell 262’s central galaxy hosts a kpc-scale disk. The nebular gas in RXJ0820.9+0752 is offset and redshifted with respect to the central galaxy by 10 − 20 kpc and 150 km s−1, respectively. The nebular gases in PKS 0745-191 and Abell 1835 are being churned to higher velocity dispersion by X-ray bubbles and jets. The churned gas is enveloped by larger scale, lower velocity dispersion (quiescent) nebular emission. The mean line-of-sight speeds of the churned gas, quiescent gas, and the central galaxy each differ by up to ∼ 150 km s−1; nebular speeds upward of 800 km s−1 are found. Gases with outwardly-rising speeds upward of several hundred km s−1 are consistent with being advected behind and being lifted by the rising bubbles. The peculiar motion between the galaxy, nebular gas, and perhaps the hot atmosphere from which it presumably condensed is affecting the bubble dynamics, and may strongly affect thermally unstable cooling, the dispersal of jet energy, and the angular momentum of gas accreting onto the galaxies and their nuclear black holes.

Citation

Gingras, M.-J., Coil, A. L., Mcnamara, B. R., Perrotta, S., Brighenti, F., Russell, H. R., Li, M., Peng Oh, S., & Wenmeng, W. (in press). Complex Velocity Structure of Nebular Gas in Active Galaxies Centred in Cooling X-ray Atmospheres. Astrophysical Journal,

Journal Article Type Article
Acceptance Date Sep 26, 2024
Deposit Date Sep 30, 2024
Publicly Available Date Oct 1, 2024
Journal Astrophysical Journal
Print ISSN 0004-637X
Electronic ISSN 1538-4357
Publisher American Astronomical Society
Peer Reviewed Peer Reviewed
Keywords Nebular Emission; X-ray Clusters; RXJ08209+0752; PKS 0745-191; Abell 1835; Abell 262
Public URL https://nottingham-repository.worktribe.com/output/40253503

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