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ULLYSES and Complementary Surveys of Massive Stars in the Magellanic Clouds

Published online by Cambridge University Press:  29 August 2024

Paul A. Crowther Open the ORCID record for Paul A. Crowther [Opens in a new window]
Paul A. Crowther*
Affiliation:
Department of Physics & Astronomy, University of Sheffield Hounsfield Road, Sheffield, S3 7RH, UK
*
email: paul.crowther@sheffield.ac.uk
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Abstract

An overview is provided of the scientific goals of the Magellanic Cloud component of the STScI Directors Discretionary UV initiative ULLYSES, together with the complementary spectroscopic survey XShootU (VLT/Xshooter) and other ancillary datasets. Together, ULLYSES and XShootU permit the first comprehensive, homogeneous study of wind densities and velocities in metal-poor massive stars, plus UV/optical spectroscopic libraries for population synthesis models and a large number of interstellar sight-lines towards the Magellanic Clouds.

Keywords

Stars: early-typeStars: massiveStars: evolutionStars: winds, outflowsStars: abundancesStars: fundamental parameters

Information

Type
Contributed Paper
Information
Proceedings of the International Astronomical Union , Volume 18 , Symposium S361: Massive Stars Near and Far , May 2022 , pp. 15 - 25
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Copyright
© The Author(s), 2024. Published by Cambridge University Press on behalf of International Astronomical Union

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