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2020MNRAS.492.2177K - Mon. Not. R. Astron. Soc., 492, 2177-2192 (2020/February-3)
How stellar rotation shapes the colour-magnitude diagram of the massive intermediate-age star cluster NGC 1846.
KAMANN S., BASTIAN N., GOSSAGE S., BAADE D., CABRERA-ZIRI I., DA COSTA G., DE MINK S.E., GEORGY C., GIESERS B., GOTTGENS F., HILKER M., HUSSER T.-O., LARDO C., LARSEN S.S., MACKEY D., MARTOCCHIA S., MUCCIARELLI A., PLATAIS I., ROTH M.M., SALARIS M., USHER C. and YONG D.
Abstract (from CDS):
Abstract Copyright: © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society
Journal keyword(s): Hertzsprung-Russell and colour-magnitude diagrams - stars: rotation - galaxies: star clusters: individual: NGC 1846
Simbad objects: 8
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