Reconciling Observed and Simulated Stellar Halo Masses

Robyn E. Sanderson, Shea Garrison-Kimmel, Andrew Wetzel, Tsang Keung Chan, Philip F. Hopkins, Dušan Kereš, Ivanna Escala, Claude André Faucher-Giguère, Xiangcheng Ma

Research output: Contribution to journalArticlepeer-review

16 Scopus citations

Abstract

We use cosmological hydrodynamical simulations of Milky Way-mass galaxies from the FIRE project to evaluate various strategies for estimating the mass of a galaxy's stellar halo from deep, integrated-light images. We find good agreement with integrated-light observations if we mimic observational methods to measure the mass of the stellar halo by selecting regions of an image via projected radius relative to the disk scale length or by their surface density in stellar mass. However, these observational methods systematically underestimate the accreted stellar component, defined in our (and most) simulations as the mass of stars formed outside of the host galaxy, by up to a factor of 10, since the accreted component is centrally concentrated and therefore substantially obscured by the galactic disk. Furthermore, these observational methods introduce spurious dependencies of the estimated accreted stellar component on the stellar mass and size of galaxies that can obscure the trends in accreted stellar mass predicted by cosmological simulations, since we find that in our simulations, the size and shape of the central galaxy are not strongly correlated with the assembly history of the accreted stellar halo. This effect persists whether galaxies are viewed edge-on or face-on. We show that metallicity or color information may provide a way to more cleanly delineate in observations the regions dominated by accreted stars. Absent additional data, we caution that estimates of the mass of the accreted stellar component from single-band images alone should be taken as lower limits.

Original languageEnglish (US)
Article number12
JournalAstrophysical Journal
Volume869
Issue number1
DOIs
StatePublished - Dec 10 2018

Keywords

  • dark matter
  • galaxies: halos
  • galaxies: structure
  • methods: numerical
  • methods: observational

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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