The Astrophysical Journal (Jan 2024)

The Cosmic Ultraviolet Baryon Survey (CUBS). VII. On the Warm-hot Circumgalactic Medium Probed by O vi and Ne viii at 0.4 ≲ z ≲ 0.7

  • Zhijie Qu,
  • Hsiao-Wen Chen,
  • Sean D. Johnson,
  • Gwen C. Rudie,
  • Fakhri S. Zahedy,
  • David DePalma,
  • Joop Schaye,
  • Erin T. Boettcher,
  • Sebastiano Cantalupo,
  • Mandy C. Chen,
  • Claude-André Faucher-Giguère,
  • Jennifer I-Hsiu Li,
  • John S. Mulchaey,
  • Patrick Petitjean,
  • Marc Rafelski

DOI
https://doi.org/10.3847/1538-4357/ad410b
Journal volume & issue
Vol. 968, no. 1
p. 8

Abstract

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This paper presents a newly established sample of 103 unique galaxies or galaxy groups at 0.4 ≲ z ≲ 0.7 from the Cosmic Ultraviolet Baryon Survey (CUBS) for studying the warm-hot circumgalactic medium (CGM) probed by both O vi and Ne viii absorption. The galaxies and associated neighbors are identified at 40 km s ^−1 for galaxies of $\mathrm{log}{M}_{\mathrm{star}}/{M}_{\odot }\gt 9$ within the virial radius, suggesting a more dynamic warm-hot halo around these galaxies. Finally, the warm-hot CGM probed by O vi and Ne viii is suggested to be the dominant phase in sub- L * galaxies with $\mathrm{log}{M}_{\mathrm{star}}/{M}_{\odot }\approx 9\mbox{--}10$ based on their high ionization fractions in the CGM.

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