The Astrophysical Journal (Jan 2023)

Investigating the Dominant Environmental Quenching Process in UVCANDELS/COSMOS Groups

  • Bonnabelle Zabelle,
  • Claudia Scarlata,
  • Vihang Mehta,
  • Harry I. Teplitz,
  • Marc Rafelski,
  • Xin Wang,
  • Ben Sunnquist,
  • Laura Prichard,
  • Norman Grogin,
  • Anton Koekemoer,
  • Rogier Windhorst,
  • Michael Rutkowski,
  • Anahita Alavi,
  • Nima Chartab,
  • Christopher J. Conselice,
  • Y. Sophia Dai,
  • Eric Gawiser,
  • Mauro Giavalisco,
  • Pablo Arrabal Haro,
  • Nimish Hathi,
  • Rolf A. Jansen,
  • Zhiyuan Ji,
  • Ray A. Lucas,
  • Kameswara Mantha,
  • Bahram Mobasher,
  • Robert W. O’Connell,
  • Brant Robertson,
  • Zahra Sattari,
  • L. Y. Aaron Yung,
  • Romeel Davé,
  • Duilia DeMello,
  • Mark Dickinson,
  • Henry Ferguson,
  • Steven L. Finkelstein,
  • Matt Hayes,
  • Justin Howell,
  • Sugata Kaviraj,
  • John W. Mackenty,
  • Brian Siana

DOI
https://doi.org/10.3847/1538-4357/acacfd
Journal volume & issue
Vol. 947, no. 1
p. 17

Abstract

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We explore how the fraction of quenched galaxies changes in groups of galaxies with respect to the distance to the center of the group, redshift, and stellar mass to determine the dominant process of environmental quenching in 0.2 10.56 group galaxies, we find that the probability of being quenched increases slowly with decreasing redshift, diverging from the stagnant field galaxy population. A corresponding analysis on how the probability of being quenched increases with time within groups suggests that the dominant environmental quenching process is characterized by slow (∼Gyr) timescales. We find a quenching time of approximately ${4.91}_{-1.47}^{+0.91}$ Gyr, consistent with the slow processes of strangulation and delayed-then-rapid quenching although more data are needed to confirm this result.

Keywords