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A 4000 Mʘ supermassive star as a possible source for the W1 kilomaser

Published online by Cambridge University Press:  07 February 2024

Katarzyna Nowak Open the ORCID record for Katarzyna Nowak [Opens in a new window]  and
Martin G. H. Krause
Katarzyna Nowak*
Affiliation:
Centre for Astrophysics Research, Department of Physics, Astronomy and Mathematics, University of Hertfordshire, College Lane, Hatfield AL10 9AB, UK.
Martin G. H. Krause
Affiliation:
Centre for Astrophysics Research, Department of Physics, Astronomy and Mathematics, University of Hertfordshire, College Lane, Hatfield AL10 9AB, UK.
*
email: k.nowak@herts.ac.uk
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Abstract

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Supermassive stars have been proposed as the solution to a number of longstanding problems in globular cluster formation. The hypothetical stars have been suggested as potential polluters responsible for the observed chemical peculiarities within those clusters. In recent hydrodynamic simulations, we have demonstrated that accretion discs around such stars are stable even with large stellar accretion and flyby rates and produce H2O kilomasers. We propose that the W1 kilomaser, associated with a super star cluster in the starburst galaxy NGC 253, may arise in an accretion disc around a supermassive star with a mass of around 4000 Mʘ.

Keywords

star clustersmasersaccretion discshydrodynamics
Type
Contributed Paper
Information
Proceedings of the International Astronomical Union , Volume 18 , Symposium S380: Cosmic Masers: Proper Motion toward the Next-Generation Large Projects , December 2022 , pp. 36 - 39
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Copyright
© The Author(s), 2024. Published by Cambridge University Press on behalf of International Astronomical Union

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