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arXiv · 1512.00253

Evidence for the rapid formation of low mass early-type galaxies in dense environments

Yiqing Liu·Eric W. Peng·John Blakeslee·Patrick Côté·Laura Ferrarese·Andrés Jordán·Thomas H. Puzia·Elisa Toloba·Hong-Xin Zhang
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Abstract

We explore the environmental dependence of star formation timescales in low mass galaxies using the [$α$/Fe] abundance ratio as an evolutionary clock. We present integrated [$α$/Fe] measurements for 11 low mass ($M_\star \sim 10^9~M_\odot$) early-type galaxies (ETGs) with a large range of cluster-centric distance in the Virgo Cluster. We find a gradient in [$α$/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 [$α$/Fe]. Galaxies in this mass range exhibit a large scatter in the [$α$/Fe]--$σ$ diagram, and do not obviously lie on an extension of the relation defined by massive ETGs. In addition, we find a correlation between [$α$/Fe] and globular cluster specific frequency ($S_N$), 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 [$α$/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-[$α$/Fe], high-$S_N$ stellar populations seen in the outer halos of massive ETGs.

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Yiqing Liu, Eric W. Peng, John Blakeslee, Patrick Côté, Laura Ferrarese, Andrés Jordán, Thomas H. Puzia, Elisa Toloba, Hong-Xin Zhang. 2015-12-01. Evidence for the rapid formation of low mass early-type galaxies in dense environments. https://doi.org/10.3847/0004-637x%2F818%2F2%2F179

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