$R_{\rm e}$. I. Understanding galaxy sizes, associated luminosity densities, and the artificial division of the early-type galaxy population
Alister W. Graham

TL;DR
This paper critically examines the use of the effective radius in early-type galaxies, revealing that the perceived division between dwarf and giant galaxies is artificial and depends on arbitrary measurement choices, impacting many related astrophysical conclusions.
Contribution
The study demonstrates that the supposed dichotomy in early-type galaxies is an artifact of measurement definitions, challenging longstanding classifications and their implications for galaxy formation theories.
Findings
The division at M_B ≈ -18 mag is artificial and measurement-dependent.
Galaxy property correlations vary with the percentage of light used to define R_e.
Implications affect dark matter estimates, galaxy formation models, and black hole studies.
Abstract
The deceptive simplicity of the radius enclosing an arbitrary 50 percent of a galaxy's light has hamstrung the understanding of early-type galaxies (ETGs). Half a century ago, using the "effective half-light radii" from de Vaucouleurs' model, S\'ersic reported that bright ETGs follow the relation ; and consequently one has that and , where and are the effective surface brightness at and the mean effective surface brightness within , respectively. S\'ersic additionally observed an apparent transition which led him to advocate for a division between what he called dwarf and giant ETGs; a belief frequently restated to occur at mag or S\'ersic . Here, the location of this false dichotomy is shown…
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