Context. The surface brightness distribution of ~30–40% of the early-type dwarf galaxies with − 18 ≤ MB ≤ −15 in the Virgo and the Coma clusters is fitted by models that include two structural components (Sérsic + exponential) as for bright disc galaxies.
No takes yet. Share an insight, caveat, or question.
J. A. L. Aguerri (2016) studied this question.
Synapse has enriched 5 related papers. Consider them for comparative context: