no code implementations • 28 Oct 2019 • Michelle L. M. Collins, Erik J. Tollerud, R. Michael Rich, Rodrigo A. Ibata, Nicolas F. Martin, Scott C. Chapman, Karoline M. Gilbert, Janet Preston
We find its mass-to-light ratio is higher than galaxies of comparable stellar mass ($[M/L]_{\rm half} = 278^{+146}_{-198}M_\odot/L_\odot$), but its dynamics place it in a halo with a similar total mass to these galaxies.
Astrophysics of Galaxies