Evidence for the rapid formation of low mass early-type galaxies in dense environments
arXiv:1512.00253 · doi:10.3847/0004-637X/818/2/179
Abstract
We explore the environmental dependence of star formation timescales in low mass galaxies using the [/Fe] abundance ratio as an evolutionary clock. We present integrated [/Fe] measurements for 11 low mass () early-type galaxies (ETGs) with a large range of cluster-centric distance in the Virgo Cluster. We find a gradient in [/Fe], where the galaxies closest to the cluster center (the cD galaxy, M87) have the highest values. This trend is driven by galaxies within a projected radius of 0.4~Mpc (0.26 times the virial radius of Virgo~A), all of which have super-solar [/Fe]. Galaxies in this mass range exhibit a large scatter in the [/Fe]-- diagram, and do not obviously lie on an extension of the relation defined by massive ETGs. In addition, we find a correlation between [/Fe] and globular cluster specific frequency (), suggesting that low-mass ETGs that formed their stars over a short period of time, were also efficient at forming massive star clusters. The innermost low-mass ETGs in our sample have [/Fe] values comparable to that of M87, implying that environment is the controlling factor for star formation timescales in dense regions. These low-mass galaxies could be the surviving counterparts of the objects that have already been accreted into the halo of M87, and may be the link between present-day low-mass galaxies and the old, metal-poor, high-[/Fe], high- stellar populations seen in the outer halos of massive ETGs.
11 pages, 8 figures
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