power-law elliptical galaxy kahkešÃ¢n-e beyzigun bâ qânun-e tavâni Fr.: galaxie elliptique en loi de puissance An → elliptical galaxy whose → surface brightness can be approximated by a single → power law at small radii (r ≤ 10-20’’). More modern interpretations have emphasized that these profiles can be better understood as the inward continuation of the galaxy’s overall → Sersic profile, usually modified by an additional, nuclear-scale stellar component (S. P. Rusli et al., 2013, AJ 146, 160). |