Spectroscopic decomposition of the galaxy and halo of the cD galaxy NGC 3311
Information on the star-formation histories of cD galaxies and their extended stellar haloes lie in their spectra. Therefore, to determine whether these structures evolved together or through a two-phase formation, we need to spectroscopically separate the light from each component. We present a pil...
| Main Authors: | , , |
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| Format: | Article |
| Published: |
Oxford University Press
2018
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| Subjects: | |
| Online Access: | https://eprints.nottingham.ac.uk/52095/ |