Under Pressure: Quenching Star Formation in Low-Mass Satellite Galaxies via Stripping

TL;DR

This study investigates how environmental effects like ram-pressure stripping quench star formation in low-mass satellite galaxies, highlighting the importance of clumpy host halo gas in matching observed gas depletion.

Contribution

It demonstrates that clumpy halo gas distributions are essential to reproduce observed quenching efficiencies in low-mass satellites, advancing understanding of environmental quenching mechanisms.

Findings

Stripping becomes effective below stellar mass 10^{8-9} M_sun.

Canonical halo densities are insufficient for full gas stripping.

Clumpy halo gas reproduces observed HI fractions and quenching timescales.

Abstract

Recent studies of galaxies in the local Universe, including those in the Local Group, find that the efficiency of environmental (or satellite) quenching increases dramatically at satellite stellar masses below ~ $10^8\ {\rm M}_{\odot}$. This suggests a physical scale where quenching transitions from a slow "starvation" mode to a rapid "stripping" mode at low masses. We investigate the plausibility of this scenario using observed HI surface density profiles for a sample of 66 nearby galaxies as inputs to analytic calculations of ram-pressure and viscous stripping. Across a broad range of host properties, we find that stripping becomes increasingly effective at $M_{*} < 10^{8-9}\ {\rm M}_{\odot}$, reproducing the critical mass scale observed. However, for canonical values of the circumgalactic medium density ($n_{\rm halo} < 10^{-3.5}$ ${\rm cm}^{-3}$), we find that stripping is not fully effective; infalling satellites are, on average, stripped of < 40 - 70% of their cold gas reservoir, which is insufficient to match observations. By including a host halo gas distribution that is clumpy and therefore contains regions of higher density, we are able to reproduce the observed HI gas fractions (and thus the high quenched fraction and short quenching timescale) of Local Group satellites, suggesting that a host halo with clumpy gas may be crucial for quenching low-mass systems in Local Group-like (and more massive) host halos.