# 'Scraggy' dark halos around bulge-less spiral galaxies

## TL;DR

This study investigates the dark matter halos of bulge-less spiral galaxies, finding they have significantly lower dark halo mass-to-light ratios compared to bulgy spirals, indicating less dark matter presence.

## Contribution

It provides the first estimate of dark halo mass-to-light ratios for bulge-less spiral galaxies using satellite orbital motions.

## Key findings

- Bulge-less spirals have low dark halo mass-to-light ratios (~20).
- Dark halos around bulge-less galaxies are about half as massive as those around bulgy spirals.
- Sample includes 220 galaxies with 43 dwarf companions and 7 in the Local Volume.

## Abstract

We use a sample of 220 face-on bulge-less galaxies situated in the low density environment to estimate their total mass via orbital motions of supposed rare satellites. Our inspection reveals 43 dwarf companions having the mean projected separation of 130 kpc and the mean-square velocity difference of 96 km/s. For them, we obtain the mean orbital-mass-to-K-band luminosity ratio of $20\pm3$. Seven bulge-less spirals in the Local Volume are also characterized by the low mean ratio, $M_{orb}/L_K = 22\pm5$. We conclude that bulge-less Sc-Scd-Sd galaxies have poor dark halos, about two times lower than that of bulgy spiral galaxies of the same stellar mass.