A Revised Parallel-Sequence Morphological Classification of Galaxies: Structure and Formation of S0 and Spheroidal Galaxies
John Kormendy, Ralf Bender

TL;DR
This paper proposes an updated galaxy classification system that includes spheroidal galaxies in parallel with irregulars, supported by structural analysis and galaxy transformation process insights.
Contribution
It introduces a revised classification extending S0 sequences to spheroidals, linking them with irregulars, and provides structural data supporting a continuous galaxy evolution sequence.
Findings
Spheroidal galaxies form a continuous sequence with S0 disks.
Sphs are structurally similar to irregular and spiral galaxy disks.
Galaxy transformation processes like ram-pressure stripping are discussed.
Abstract
We update van den Bergh's parallel sequence galaxy classification in which S0 galaxies form a sequence S0a-S0b-S0c that parallels the sequence Sa-Sb-Sc of spiral galaxies. The ratio B/T of bulge to total light defines the position of a galaxy in each sequence. Our classification makes one improvement. We extend the S0a-S0b-S0c sequence to spheroidal ("Sph'") galaxies that are positioned in parallel to irregular galaxies in a similarly extended Sa-Sb-Sc-Im sequence. This provides a natural "home" for spheroidals, which previously were omitted from galaxy classifications. To motivate our juxtaposition of Sph and irregular galaxies, we present photometry and bulge-disk decompositions of Virgo S0s, including late-type S0s that bridge the gap between S0b and Sph galaxies. NGC 4762 is a SB0bc with B/T = 0.13. NGC 4452 is a SB0c galaxy with an even tinier pseudobulge. VCC 2048 and NGC 4638…
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