# ALMA observations of molecular gas in the host galaxy of AT2018cow

**Authors:** Kana Morokuma-Matsui, Tomoki Morokuma, Nozomu Tominaga, Bunyo, Hatsukade, Masao Hayashi, Yoichi Tamura, Yuichi Matsuda, Kazuhito Motogi,, Kotaro Niinuma, and Masahiro Konishi

arXiv: 1906.05446 · 2019-07-10

## TL;DR

This study uses ALMA data to analyze the molecular gas and star formation in the host galaxy of AT2018cow, revealing it as a typical star-forming dwarf galaxy with implications for FELT progenitors.

## Contribution

First molecular gas analysis of a FELT host galaxy, showing its star-forming nature and potential link to massive star explosions.

## Key findings

- Detected CO emission indicating molecular gas mass of 1.85e8 M_sun
- Located at a star-forming region with a blue star cluster
- Host galaxy has solar or super-solar metallicity

## Abstract

We investigate the molecular gas in, and star-formation properties of, the host galaxy (CGCG 137-068) of a mysterious transient, AT2018cow, at kpc and larger scales, using archival band-3 data from the Atacama Large Millimeter/submillimeter Array (ALMA). AT2018cow is the nearest Fast-Evolving Luminous Transient (FELT), and this is the very first study unveiling molecular-gas properties of FELTs. The achieved rms and beam size are 0.21 mJy beam$^{-1}$ at a velocity resolution of $40$ km s$^{-1}$ and $3".66\times2".71$ ($1.1~{\rm kpc} \times 0.8~{\rm kpc}$), respectively. CO($J$=1-0) emission is successfully detected. The total molecular gas mass inferred from the CO data is $(1.85\pm0.04)\times10^8$ M$_\odot$ with the Milky Way CO-to-H$_2$ conversion factor. The H$_2$ column density at the AT2018cow site is estimated to be $8.6\times10^{20}$ cm$^{-2}$. The ALMA data reveal that (1) CGCG 137-068 is a normal star-forming (SF) dwarf galaxy in terms of its molecular gas and star-formation properties and (2) AT2018cow is located between a CO peak and a blue star cluster. These properties suggest on-going star formation and favor the explosion of a massive star as the progenitor of AT2018cow. We also find that CGCG 137-068 has a solar or super-solar metallicity. If the metallicity of the other FELT hosts is not higher than average, then some property of SF dwarf galaxies other than metallicity may be related to FELTs.

## Full text

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## Figures

3 figures with captions in the complete paper: https://tomesphere.com/paper/1906.05446/full.md

## References

47 references — full list in the complete paper: https://tomesphere.com/paper/1906.05446/full.md

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Source: https://tomesphere.com/paper/1906.05446