# ALMA and HST kiloparsec-scale imaging of a quasar-galaxy merger at   $z\approx 6.2$

**Authors:** Roberto Decarli, Massimo Dotti, Eduardo Ba\~nados, Emanuele Paolo, Farina, Fabian Walter, Chris Carilli, Xiaohui Fan, Chiara Mazzucchelli,, Marcel Neeleman, Mladen Novak, Dominik Riechers, Michael A. Strauss, Bram P., Venemans, Yujin Yang, Ran Wang

arXiv: 1906.05308 · 2019-08-14

## TL;DR

This study presents high-resolution ALMA and HST imaging of a quasar-galaxy merger at redshift 6.2, revealing detailed structures, gas dynamics, and star formation activity during the early universe.

## Contribution

First detailed kpc-scale imaging of a quasar-galaxy merger at cosmic dawn, showing multiple components and tidal interactions at z~6.2.

## Key findings

- Resolved multiple galaxy components with dust, gas, and UV emission.
- Observed high-velocity [CII] emission over 1500 km/s.
- Identified tidal features consistent with a satellite galaxy.

## Abstract

We present kpc-scale ALMA and HST imaging of the quasar PJ308-21 at $z$=$6.2342$, tracing dust, gas (via the [CII] 158 $\mu$m line) and young stars. At a resolution of $\sim0.3''$ ($\approx1.7$ kpc), the system is resolved over $>4''$ ($>$20 kpc). In particular, it features a main component, identified to be the quasar host galaxy, centered on the accreting supermassive black hole; and two other extended components on the West and East side, one redshifted and the other blueshifted relative to the quasar. The [CII] emission of the entire system stretches over $>$1500 km/s along the line of sight. All the components of the system are observed in dust, [CII], and rest-frame UV emission. The inferred [CII] luminosities [(0.9-4.6)$\times 10^9$ L$_\odot$], dust luminosities [(0.15-2.6)$\times10^{12}$ L$_\odot$], and rest-frame UV luminosities [(6.6-15)$\times10^{10}$ L$_\odot$], their ratios, and the implied gas/dust masses and star formation rates [11-290 M$_\odot$ yr$^{-1}$] are typical of high-redshift star-forming galaxies. A toy model of a single satellite galaxy that is tidally stripped by the interaction with the quasar host galaxy can account for the observed velocity and spatial extent of the two extended components. An outflow interpretation of the unique features in PJ308-21 is not supported by the data. PJ308-21 is thus one of the earliest galaxy mergers imaged at cosmic dawn.

## Full text

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## Figures

15 figures with captions in the complete paper: https://tomesphere.com/paper/1906.05308/full.md

## References

48 references — full list in the complete paper: https://tomesphere.com/paper/1906.05308/full.md

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Source: https://tomesphere.com/paper/1906.05308