Deep Extragalactic VIsible Legacy Survey (DEVILS): The emergence of bulges and decline of disk growth since $z = 1$
Abdolhosein Hashemizadeh, Simon P. Driver, Luke J. M. Davies, Aaron S., G. Robotham, Sabine Bellstedt, Rogier A. Windhorst, Matt Jarvis, Benne W., Holwerda, Malgorzata Siudek, Caroline Foster, Steven Phillipps, Jessica E., Thorne, Christian Wolf

TL;DR
This study analyzes galaxy structures from redshift 0 to 1, revealing that disks dominate stellar mass density early on, but spheroids like ellipticals and bulges grow significantly, indicating a shift from disk growth to spheroid formation over 8 billion years.
Contribution
It provides a comprehensive structural analysis of galaxies over time, highlighting the emergence and growth of spheroids and the decline of disk dominance since redshift 1.
Findings
Disks contribute ~60% of stellar mass density at z=0.8, dropping to ~30% at z=0.
Massive ellipticals increase from 20% to 30% of total stellar mass density, doubling in mass.
Growth of spheroids surpasses disk growth, indicating a shift in galaxy evolution pathways.
Abstract
We present a complete structural analysis of the ellipticals (E), diffuse bulges (dB), compact bulges (cB), and disks (D) within a redshift range , and stellar mass volume-limited sample drawn from the combined DEVILS and HST-COSMOS region. We use the {\sc ProFit} code to profile over galaxies for which visual classification into single or double-component was predefined in Paper-I. Over this redshift range, we see a growth in the total stellar mass density (SMD) of a factor of 1.5. At all epochs we find that the dominant structure, contributing to the total SMD, is the disk, and holds a fairly constant share of of the total SMD from to , dropping to at (representing decline in the total disk SMD). Other classes (E, dB, and cB) show steady growth in…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research · Astrophysics and Star Formation Studies
