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arXiv · 1703.02042

Spectroscopy of Ultra-diffuse Galaxies in the Coma Cluster

Jennifer Kadowaki·Dennis Zaritsky·R. L. Donnerstein
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Abstract

We present spectra of 5 ultra-diffuse galaxies (UDGs) in the vicinity of the Coma Cluster obtained with the Multi-Object Double Spectrograph on the Large Binocular Telescope. We confirm 4 of these as members of the cluster, quintupling the number of spectroscopically confirmed systems. Like the previously confirmed large (projected half light radius $>$ 4.6 kpc) UDG, DF44, the systems we targeted all have projected half light radii $> 2.9$ kpc. As such, we spectroscopically confirm a population of physically large UDGs in the Coma cluster. The remaining UDG is located in the field, about $45$ Mpc behind the cluster. We observe Balmer and Ca II H \& K absorption lines in all of our UDG spectra. By comparing the stacked UDG spectrum against stellar population synthesis models, we conclude that, on average, these UDGs are composed of metal-poor stars ([Fe/H] $\lesssim -1.5$). We also discover the first UDG with [OII] and [OIII] emission lines within a clustered environment, demonstrating that not all cluster UDGs are devoid of gas and sources of ionizing radiation.

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Jennifer Kadowaki, Dennis Zaritsky, R. L. Donnerstein. 2017-03-06. Spectroscopy of Ultra-diffuse Galaxies in the Coma Cluster. https://doi.org/10.3847/2041-8213%2Faa653d

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