Probing the Impact of Radio-mode Feedback on the Properties of the Cool Circumgalactic Medium

Abstract We explore the influence of radio-mode feedback on the properties of the cool circumgalactic medium (CGM). To this end, we assemble a statistical sample of approximately 30,000 radio galaxies with background quasars by combining optical spectroscopic measurements of luminous red galaxies and quasars from the year 1 data set of the Dark Energy Spectroscopic Instrument and radio sources from the LOw-Frequency ARray Two-metre Sky Survey (LoTSS) DR2 catalog and the Very Large Array Sky Survey (VLASS) quick-look catalog. Galaxies with similar optical properties but with no radio counterparts in LoTSS and VLASS are selected as the control group. We measure the cool CGM properties of radio galaxies and their control samples traced by Mg ii absorption lines, including covering fraction, rest equivalent width, and gas kinematics. Our results show no significant difference in the properties of gas around radio galaxies and their control sample, indicating that the operating radio-mode feedback of massive galaxies does not produce detectable effects on the properties of the cool CGM. Finally, we show that the CGM of radio galaxies contains a nonnegligible amount of cool gas with approximately 10 10 M ⊙ . This abundance can place a stringent constraint on the radio-mode feedback models.

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Publication Details

Journal
The Astrophysical Journal
Published
2024-10-01
DOI
https://doi.org/10.3847/1538-4357/ad6c44
Citations
5
Primary Topic
Galaxies: Formation, Evolution, Phenomena
Type
article
Field-Weighted Citation Impact
1.66

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article

Probing the Impact of Radio-mode Feedback on the Properties of the Cool Circumgalactic Medium

Ting-Wen Lan, M. Schubnell, Abhijeet Anand, D. Brooks et al.
5 citations
The Astrophysical Journal
Galaxies: Formation, Evolution, Phenomena
1.66
article

Probing the Impact of Radio-mode Feedback on the Properties of the Cool Circumgalactic Medium

Ting-Wen Lan, M. Schubnell, Abhijeet Anand, D. Brooks, Paul Martini, A. Lambert, A. D. Myers, S. Juneau, Gregory Tarlé, Jason Xavier Prochaska, L. Napolitano, Laurent Le Guillou, Axel de la Macorra, Martin Landriau, Jundan Nie, Marc Manera, J. Aguilar, J. Guy, Eusebio Sanchez, Satya Gontcho A Gontcho, B. A. Weaver, Arjun T. Dey, Steven P. Ahlen, Aaron Meisner, R. Miquel, Theodore S. Kisner, Y. L. Chang, Mehdi Rezaie, John Moustakas, Claire Poppett, Hee‐Jong Seo, Hu Zou, Graziano Rossi, Peter Doel, T. Claybaugh, D. Sprayberry
article en
5 citations

Abstract

Abstract We explore the influence of radio-mode feedback on the properties of the cool circumgalactic medium (CGM). To this end, we assemble a statistical sample of approximately 30,000 radio galaxies with background quasars by combining optical spectroscopic measurements of luminous red galaxies and quasars from the year 1 data set of the Dark Energy Spectroscopic Instrument and radio sources from the LOw-Frequency ARray Two-metre Sky Survey (LoTSS) DR2 catalog and the Very Large Array Sky Survey (VLASS) quick-look catalog. Galaxies with similar optical properties but with no radio counterparts in LoTSS and VLASS are selected as the control group. We measure the cool CGM properties of radio galaxies and their control samples traced by Mg ii absorption lines, including covering fraction, rest equivalent width, and gas kinematics. Our results show no significant difference in the properties of gas around radio galaxies and their control sample, indicating that the operating radio-mode feedback of massive galaxies does not produce detectable effects on the properties of the cool CGM. Finally, we show that the CGM of radio galaxies contains a nonnegligible amount of cool gas with approximately 10 10 M ⊙ . This abundance can place a stringent constraint on the radio-mode feedback models.

The Astrophysical JournalVol. 974(2)
Boston University (US), Institució Catalana de Recerca i Estudis Avançats (ES), Universidad Complutense de Madrid (ES), Universitat Autònoma de Barcelona (ES), University of Wyoming (US), Centre National de la Recherche Scientifique (FR), Lawrence Berkeley National Laboratory (US), Kavli Institute for the Physics and Mathematics of the Universe (JP), National Taiwan University (TW), University of California, Santa Cruz (US), Institute for High Energy Physics (ES), Kansas State University (US), Chinese Academy of Sciences (CN), University of Michigan (US), Sejong University (KR), Sorbonne Université (FR), Laboratoire de Physique Nucléaire et de Hautes Énergies (FR), Ohio University (US), Institut National de Physique Nucléaire et de Physique des Particules (FR), Community Science and Data Center (US), NSF NOIRLab (US), National Astronomical Observatories (CN), Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (ES), University College London (GB), The Ohio State University (US), Universidad Nacional Autónoma de México (MX), Siena College (US), University of California, Berkeley (US)
Ministry of Education, India, National Taiwan University, National Science and Technology Council
Openalex Percentile: Top 16%
Galaxies: Formation, Evolution, Phenomena
1.66
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