| Publication |
A high fraction of Be stars in young massive clusters: evidence for a large population of near-critically rotating stars, Bastian, N.,Cabrera-Ziri, I.,Niederhofer, F., Monthly Notices of the Royal Astronomical Society, 465, 2017-03-01 00:00:00, 2017MNRAS.465.4795B||Multiple stellar populations in Magellanic Cloud clusters - III. The first evidence of an extended main sequence turn-off in a young cluster: NGC 1856, Milone, A. P.,Bedin, L. R.,Piotto, G., Monthly Notices of the Royal Astronomical Society, 450, 2015-07-01 00:00:00, 2015MNRAS.450.3750M||Multiple stellar populations in Magellanic Cloud clusters - VI. A survey of multiple sequences and Be stars in young clusters, Milone, A. P.,Marino, A. F.,Di Criscienzo, M., Monthly Notices of the Royal Astronomical Society, 477, 2018-06-01 00:00:00, 2018MNRAS.477.2640M||New constraints on the star formation history of the star cluster NGC 1856, Correnti, Matteo,Goudfrooij, Paul,Puzia, Thomas H., Monthly Notices of the Royal Astronomical Society, 450, 2015-07-01 00:00:00, 2015MNRAS.450.3054C||The Radial Distributions of the Two Main-sequence Components in the Young Massive Star Cluster NGC 1856, Li, Chengyuan,de Grijs, Richard,Deng, Licai, The Astrophysical Journal, 834, 2017-01-01 00:00:00, 2017ApJ...834..156L||The young massive SMC cluster NGC 330 seen by MUSE. II. Multiplicity properties of the massive-star population, Bodensteiner, Julia,Sana, Hugues,Wang, Chen, Astronomy and Astrophysics, 652, 2021-08-01 00:00:00, 2021A&A...652A..70B |
