# Galaxy Rotation Coherent with the Motions of Neighbors: Discovery of   Observational Evidence

**Authors:** Joon Hyeop Lee, Mina Pak, Hye-Ran Lee, Hyunmi Song

arXiv: 1901.02151 · 2019-02-20

## TL;DR

This study provides observational evidence that galaxy rotation is coherently aligned with the motions of neighboring galaxies within 800 kpc, highlighting the influence of interactions on galaxy kinematics.

## Contribution

First observational detection of dynamical coherence between galaxy rotation and neighbor motions using CALIFA and NSA data.

## Key findings

- Significant velocity coherence within 800 kpc, up to 61.7 km/s.
- Stronger coherence observed in faint, blue, or misaligned galaxies.
- Galaxy interactions influence internal kinematic structures.

## Abstract

We present our discovery of observational evidence for the coherence between galaxy rotation and the average line-of-sight motion of neighbors. We use the Calar Alto Legacy Integral Field Area (CALIFA) survey data analyzed with the Python CALIFA STARLIGHT Synthesis Organizer (PyCASSO) platform, and the NASA-Sloan Atlas (NSA) catalog. After estimating the projected angular momentum vectors of 445 CALIFA galaxies, we build composite maps of their neighbor galaxies on the parameter space of line-of-sight velocity versus projected distance. The composite radial profiles of the luminosity-weighted mean velocity of neighbors show striking evidence for dynamical coherence between the rotational direction of the CALIFA galaxies and the average moving direction of their neighbor galaxies. The signal of such dynamical coherence is significant for the neighbors within 800 kpc distance from the CALIFA galaxies, for which the luminosity-weighted mean velocity is as large as 61.7+/-17.6 km/s (3.5-sigma significance to bootstrap uncertainty) when the angular momentum is measured at R_e<R<=2R_e of each CALIFA galaxy. In the comparison of the subsamples, we find that faint, blue or kinematically misaligned galaxies show stronger coherence with neighbor motions than bright, red or kinematically well-aligned galaxies do. Our results indicate that (1) the rotation of a galaxy (particularly at its outskirt) is significantly influenced by interactions with its neighbors up to 800 kpc, (2) the coherence is particularly strong between faint galaxies and bright neighbors, and (3) galaxy interactions often cause internal kinematic misalignment or possibly even kinematically distinct cores.

## Full text

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## Figures

39 figures with captions in the complete paper: https://tomesphere.com/paper/1901.02151/full.md

## References

65 references — full list in the complete paper: https://tomesphere.com/paper/1901.02151/full.md

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Source: https://tomesphere.com/paper/1901.02151