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MUSE 3D spectroscopy of BA-type supergiants in NGC 300

Gonzalez-Tora, G, Urbaneja, MA, Przybilla, N, Dreizler, S, Roth, MM, Kamann, S and Castro, N MUSE 3D spectroscopy of BA-type supergiants in NGC 300. In: IAU Symposia IAUS 361: Massive Stars Near and Far (361). (IAUS 361: Massive Stars Near & Far, Ireland). (Accepted)

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We present the results obtained using spectroscopic data taken with the intermediateresolution Multi Unit Spectroscopic Explorer (MUSE) of B and A-type supergiants and bright giants in the Sculptor Group galaxy NGC 300. For our analysis, a hybrid local thermodynamic equilibrium (LTE) line-blanketing+non-LTE method was used to improve the previously published results for the same data. In addition, we present some further applications of this work, which includes extending the flux-weighted gravity luminosity relationship (FGLR), a distance determination method for supergiants. This pioneering work opens up a new window to explore this relation, and also demonstrates the enormo

Item Type: Conference or Workshop Item (Paper)
Uncontrolled Keywords: astro-ph.SR; astro-ph.SR; astro-ph.GA
Subjects: Q Science > QB Astronomy
Q Science > QC Physics
Divisions: Astrophysics Research Institute
Publisher: Cambridge University Press (CUP)
Related URLs:
SWORD Depositor: A Symplectic
Date Deposited: 10 Oct 2022 08:22
Last Modified: 10 Oct 2022 08:22
URI: https://researchonline.ljmu.ac.uk/id/eprint/17758
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