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- W1524982503 abstract "The circumnuclear starburst of M83 (NGC 5236), the nearest such example (4.6 Mpc), constitutes an ideal site for studying the massive star IMF at high metallicity (12+log[O/H]=9.1$pm$0.2, Bresolin & Kennicutt 2002). We analyzed archival HST/STIS FUV imaging and spectroscopy of 13 circumnuclear star clusters in M83. We compared the observed spectra with two types of single stellar population (SSP) models, semi-empirical models, which are based on an empirical library of Galactic O and B stars observed with IUE (Robert et al. 1993), and theoretical models, which are based on a new theoretical UV library of hot massive stars described in Leitherer et al. (2010) and computed with WM-Basic (Pauldrach et al. 2001). The models were generated with Starburst99 (Leitherer & Chen 2009). We derived the reddenings, the ages, and the masses of the clusters from model fits to the FUV spectroscopy, as well as from optical HST/WFC3 photometry." @default.
- W1524982503 created "2016-06-24" @default.
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- W1524982503 date "2010-11-15" @default.
- W1524982503 modified "2023-10-14" @default.
- W1524982503 title "The Massive Star Content of Circumnuclear Star Clusters in M83" @default.
- W1524982503 doi "https://doi.org/10.48550/arxiv.1011.3476" @default.
- W1524982503 hasPublicationYear "2010" @default.
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