The black hole in the most massive ultracompact dwarf galaxy M59-UCD3
We examine the internal properties of the most massive ultracompact dwarf galaxy (UCD), M59-UCD3, by combining adaptive-optics-assisted near-IR integral field spectroscopy from Gemini/NIFS and Hubble Space Telescope (HST) imaging. We use the multiband HST imaging to create a mass model that suggests...
| Main Authors: | , , , |
|---|---|
| Format: | Journal article |
| Published: |
American Astronomical Society
2018
|