http://arxiv.org/abs/1705.08513
We present Hubble Space Telescope imaging of two ultra diffuse galaxies (UDGs) with measured stellar velocity dispersions in the Coma cluster. The galaxies, Dragonfly 44 and DFX1, have effective radii of 4.7 kpc and 3.5 kpc and velocity dispersions of $47^{+8}{-6}$ km/s and $30^{+7}{-7}$ km/s, respectively. Both galaxies are associated with a striking number of compact objects, tentatively identified as globular clusters: $N_{\rm gc}=74\pm 18$ for Dragonfly 44 and $N_{\rm gc}=62\pm 17$ for DFX1. The number of globular clusters is far higher than expected from the luminosities of the galaxies but is consistent with expectations from the empirical relation between dynamical mass and globular cluster count defined by other galaxies. Combining our data for these two objects with previous HST observations of Coma UDGs we find that most have large globular cluster populations for their luminosities, in contrast to a recent study of a similar sample by Amorisco et al. (2017), but consistent with earlier results for individual galaxies. The Harris et al. (2017) relation between globular cluster count and dark matter halo mass implies a median halo mass of $M_{\rm halo}\sim 1.5\times 10^{11}\,{\rm M}{\odot}$ for the sixteen Coma UDGs that have been observed with HST so far, with the largest and brightest having $M{\rm halo}\sim 5\times 10^{11}\,{\rm M}_{\odot}$.
P. Dokkum, R. Abraham, A. Romanowsky, et. al.
Thu, 25 May 17
16/44
Comments: Submitted to ApJ Letters. The black and white panels of Figure 1 make the key point of the paper, hopefully