Abstract
Recent results of CASPECtroscopic abundance determinations of B stars in the Magellanic Clouds (MCs) are presented. The sample stars include both young globular cluster (NGC 1818, 2004 (both LMC), 330 (SMC)) and field stars on and close to the main sequence (MS). They were selected to be slow projected rotators (v sin i < 75 km/s) and non-Be stars (no emission in Hα). The spectra have R = 20 000, a S/N of around 100 and a range of 4000 to 5000 Å in wavelength.
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© 1999 Springer-Verlag Berlin Heidelberg
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Korn, A.J., Wolf, B. (1999). NLTE Analyses of Magellanic Cloud B Stars. In: Walsh, J.R., Rosa, M.R. (eds) Chemical Evolution from Zero to High Redshift. ESO Astrophysics Symposia. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-48360-1_27
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DOI: https://doi.org/10.1007/978-3-540-48360-1_27
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-662-21697-2
Online ISBN: 978-3-540-48360-1
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