Could kilomasers pinpoint supermassive stars?
Katarzyna Nowak, Martin. G. H. Krause, Daniel Schaerer

TL;DR
This study explores whether kilomasers can be used to identify supermassive stars by modeling their accretion discs and comparing simulated maser spectra with observed data, supporting the hypothesis that kilomasers can pinpoint such stars.
Contribution
The paper presents hydrodynamic simulations of accretion discs around supermassive stars and compares the resulting maser spectra with observations, suggesting kilomasers as indicators of supermassive stars.
Findings
Model discs survive in dynamic environments.
Simulated spectra match observed kilomaser W1 reasonably well.
Stars of a few thousand solar masses fit the data better.
Abstract
A strong nuclear kilomaser, W1, has been found in the nearby galaxy NGC 253, associated with a forming super star cluster. Kilomasers could arise from the accretion disc around supermassive stars (>10^3 Msun), hypothetical objects that have been proposed as polluters responsible for the chemical peculiarities in globular clusters. The supermassive stars would form via runaway collisions, simultaneously with the cluster. Their discs are perturbed by stellar flybys, inspiralling and colliding stars. This raises the question if an accretion disc would at all be able to survive in such a dynamic environment and mase water lines. We investigated what the predicted maser spectrum of such a disc would look like using 2D hydrodynamic simulations and compared this to the W1 kilomaser. We derived model maser spectra from the simulations by using a general maser model for appropriate disc…
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