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

Journal Article · · The Astrophysical Journal
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  1. National Taiwan University, Taipei (Taiwan)
  2. University of California, Santa Cruz, CA (United States); Kavli Institute for the Physics and Mathematics of the Universe, Kashiwa (Japan)
  3. University of Wyoming, Laramie, WY (United States)
  4. Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)
  5. Boston University, MA (United States)
  6. University College London (United Kingdom)
  7. Universidad Nacional Autónoma de México (Mexico)
  8. NSF NOIRLab, Tucson, AZ (United States)
  9. Sorbonne Université, Paris (France)
  10. Universitat Autònoma de Barcelona, Bellaterra (Barcelona) (Spain)
  11. The Ohio State University, Columbus, OH (United States)
  12. Institut de Física d’Altes Energies (IFAE), Bellaterra Barcelona (Spain); Institució Catalana de Recerca i Estudis Avançats, Barcelona (Spain)
  13. Siena College, Loudonville, NY (United States)
  14. Chinese Academy of Sciences, Beijing (China)
  15. Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States); University of California, Berkeley, CA (United States)
  16. Kansas State University, Manhattan, KS (United States)
  17. Sejong University, Seoul (Korea, Republic of)
  18. CIEMAT, Madrid (Spain)
  19. University of Michigan, Ann Arbor, MI (United States)
  20. Ohio University, Athens, OH (United States)

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 1010M. This abundance can place a stringent constraint on the radio-mode feedback models.

Research Organization:
Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States); University of Michigan, Ann Arbor, MI (United States)
Sponsoring Organization:
Ministry of Education; National Taiwan University; U.S. National Science Foundation (NSF), Division of Astronomical Sciences; USDOE Office of Science (SC), Basic Energy Sciences (BES). Scientific User Facilities (SUF); USDOE Office of Science (SC), High Energy Physics (HEP)
Grant/Contract Number:
AC02-05CH11231; SC0019193
OSTI ID:
2891704
Journal Information:
The Astrophysical Journal, Journal Name: The Astrophysical Journal Journal Issue: 2 Vol. 974; ISSN 0004-637X; ISSN 1538-4357
Publisher:
IOP PublishingCopyright Statement
Country of Publication:
United States
Language:
English