Structure and Formation of Elliptical and Spheroidal Galaxies
John Kormendy, David B. Fisher, Mark E. Cornell, Ralf Bender

TL;DR
This study analyzes the structure of elliptical and spheroidal galaxies in the Virgo cluster, confirming their distinct formation processes and identifying new features related to their core properties and merger histories.
Contribution
It provides new surface photometry data, confirms the E-Spheroid dichotomy, and introduces the concept of extra light in coreless ellipticals linked to wet mergers.
Findings
Elliptical galaxies form a tight sequence in Fundamental Plane space.
Core ellipticals have cuspy cores, while fainter ones do not.
Coreless ellipticals show extra light at their centers.
Abstract
New surface photometry of all known elliptical galaxies in the Virgo cluster is added to published data to derive composite profiles over large dynamic ranges. Sersic functions fit them remarkably well. Effective brightnesses and radii are derived via Sersic fits and by integrating the profiles nonparametrically. We strongly confirm two dichotomies: (1) Elliptical galaxies from cDs to M32 form a tight sequence in Fundamental Plane parameter space that is almost perpendicular to the sequence of spheroidal galaxies from NGC 205 to Draco. This is consistent with our understanding of their different formation processes: mergers for Es and conversion of late-type galaxies into spheroidals by environmental effects and by energy feedback from supernovae. (2) Ellipticals come in two varieties: e.g., our 10 brightest Es have cuspy cores; our 17 fainter Es do not have cores. We find a new…
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