The universal rotation curve of low surface brightness galaxies IV: the interrelation between dark and luminous matter
Chiara Di Paolo, Paolo Salucci, Adnan Erkurt

TL;DR
This study analyzes the rotation curves of low surface brightness galaxies to understand the interplay between dark and luminous matter, revealing a universal pattern and new scaling relations that connect their structural properties.
Contribution
It introduces a detailed mass modeling approach for LSB galaxies, highlighting the role of dark matter and proposing the stellar compactness as a key parameter in the universal rotation curve.
Findings
Dark matter dominates in less luminous LSB galaxies.
Dark matter halos have a consistent central surface density across galaxy types.
A new luminous parameter, stellar compactness, is essential for modeling rotation curves.
Abstract
We investigate the properties of the baryonic and the dark matter components in low surface brightness (LSB) disc galaxies, with central surface brightness in the B band . The sample is composed by 72 objects, whose rotation curves show an orderly trend reflecting the idea of a universal rotation curve (URC) similar to that found in the local high surface brightness (HSB) spirals in previous works. This curve relies on the mass modelling of the coadded rotation curves, involving the contribution from an exponential stellar disc and a Burkert cored dark matter halo. We find that the dark matter is dominant especially within the smallest and less luminous LSB galaxies. Dark matter halos have a central surface density , similar to galaxies of different Hubble types and luminosities. We find various scaling…
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.
