The (Anti-)Hierarchical Evolution of Disk Galaxies
Asmus Boehm, Bodo L. Ziegler

TL;DR
This study uses spectroscopy and imaging to analyze over 200 spiral galaxies across redshifts 0.1 to 1.0, revealing that while total mass growth aligns with hierarchical models, stellar populations evolve anti-hierarchically, especially in low-mass galaxies.
Contribution
It provides observational evidence of anti-hierarchical stellar population evolution within the hierarchical framework of galaxy formation.
Findings
Stellar to total mass ratio remains roughly constant over time.
Low-mass spirals show stronger evolution in mass-to-light ratios than high-mass spirals.
Supports the 'down-sizing' scenario in galaxy evolution.
Abstract
Utilizing spatially resolved VLT/FORS spectroscopy and HST/ACS imaging, we constructed a sample of over 200 field spiral galaxies at redshifts 0.1<z<1.0. We find that the ratio between stellar and total mass remains roughly constant over the observed epochs, in compliance with the framework of hierarchical structure growth. However, the stellar mass-to-light ratios evolve more strongly in low-mass spirals than in high--mass spirals, indicating an anti-hierarchical evolution of their stellar populations (aka "down-sizing").
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsAstronomy and Astrophysical Research · Galaxies: Formation, Evolution, Phenomena · Stellar, planetary, and galactic studies
