RHAPSODY-G simulations: Galaxy clusters as baryonic closed boxes and the covariance between hot gas and galaxies

Hao Yi Wu, August E. Evrard, Oliver Hahn, Davide Martizzi, Romain Teyssier, Risa H. Wechsler

Research output: Contribution to journalArticlepeer-review

32 Scopus citations

Abstract

Within a sufficiently large cosmic volume, conservation of baryons implies a simple 'closed box' view in which the sum of the baryonic components must equal a constant fraction of the total enclosed mass. We present evidence from RHAPSODY-G hydrodynamic simulations of massive galaxy clusters that the closed-box expectation may hold to a surprising degree within the interior, non-linear regions of haloes. At a fixed halo mass, we find a significant anti-correlation between hot gas mass fraction and galaxy mass fraction (cold gas + stars), with a rank correlation coefficient of -0.69 within R500c. Because of this anti-correlation, the total baryon mass serves as a low-scatter proxy for total cluster mass. The fractional scatter of total baryon fraction scales approximately as 0.02(▵c/100)0.6, while the scatter of either gas mass or stellar mass is larger in magnitude and declines more slowly with increasing radius. We discuss potential observational tests using cluster samples selected by optical and hot gas properties; the simulations suggest that joint selection on stellar and hot gas has potential to achieve 5 per cent scatter in total halo mass.

Original languageEnglish (US)
Pages (from-to)1982-1991
Number of pages10
JournalMonthly Notices of the Royal Astronomical Society
Volume452
Issue number2
DOIs
StatePublished - Feb 11 2015
Externally publishedYes

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Keywords

  • Cosmology: theory
  • Galaxies: clusters: general
  • Methods: numerical
  • X-rays: galaxies: clusters

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