DOI: 10.1017/s1743921322004136 ISSN: 1743-9213

Are VMS Needed to Explain the Extreme Broad He II Emission of NGC3125-A1?

A. Wofford, A. Sixtos
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Abstract

We use HST COS G130M + G160M observations of high-z super star cluster template NGC 3125-A1 to show how the improved formulation of stellar mass loss rates has helped improve population synthesis models.

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