The Galaxy End Sequence
Stephen Eales, Pieter de Vis, Matthew Smith, Kiran Appah, Laure, Ciesla, Chris Duffield, Simon Schofield

TL;DR
This paper analyzes the distribution of galaxies in the SSFR versus stellar mass diagram, revealing a continuous, curved galaxy sequence rather than two distinct populations, and challenges the traditional dichotomy of galaxy types.
Contribution
It demonstrates that galaxies form a continuous, curved sequence in SSFR-stellar mass space, questioning the existence of a clear division between star-forming and passive galaxies.
Findings
Galaxies follow a strongly curved, extended GMS with a steep slope at high masses.
No clear morphological break exists along the galaxy sequence.
The red sequence results from color changes below a critical SSFR, not a distinct population.
Abstract
A common assumption is that galaxies fall in two distinct regions on a plot of specific star-formation rate (SSFR) versus galaxy stellar mass: a star-forming Galaxy Main Sequence (GMS) and a separate region of `passive' or `red and dead galaxies'. Starting from a volume-limited sample of nearby galaxies designed to contain most of the stellar mass in this volume, and thus being a fair representation of the Universe at the end of 12 billion years of galaxy evolution, we investigate the distribution of galaxies in this diagram today. We show that galaxies follow a strongly curved extended GMS with a steep negative slope at high galaxy stellar masses. There is a gradual change in the morphologies of the galaxies along this distribution, but there is no clear break between early-type and late-type galaxies. Examining the other evidence that there are two distinct populations, we argue that…
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