ALMA observations of molecular gas in the host galaxy of AT2018cow
arXiv:1906.05446 · doi:10.3847/2041-8213/ab2915
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 at a velocity resolution of km s and (), respectively. CO(=1-0) emission is successfully detected. The total molecular gas mass inferred from the CO data is M with the Milky Way CO-to-H conversion factor. The H column density at the AT2018cow site is estimated to be cm. 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.
8 pages, 3 figures, 2 tables, accepted for publication in ApJL
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- An environmental analysis of the fast transient AT2018cow and implications for its progenitor and late-time brightness
- A possible 250-second X-ray quasi-periodicity in the fast blue optical transient AT2018cow
- Late-time Hubble Space Telescope Observations of AT 2018cow. I. Further Constraints on the Fading Prompt Emission and Thermal Properties 50--60 Days Post-discovery
- Real-time Discovery of AT2020xnd: A Fast, Luminous Ultraviolet Transient with Minimal Radioactive Ejecta
- Spatially Resolved Molecular Gas Properties of Host Galaxy of Type I Superluminous Supernova SN 2017egm
- The interstellar medium in the environment of the supernova-less long-duration GRB 111005A
- Diverse Properties of Molecular Gas in the Host Galaxies of Fast Radio Bursts