[L99] n5236-502 , the SIMBAD biblio

[L99] n5236-502 , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.18CEST20:29:48


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Title First 3 Authors
2004A&A...427..495L 15 30 Dynamical mass estimates for two luminous young stellar clusters in Messier 83. LARSEN S.S. and RICHTLER T.
2005MNRAS.361..311D 57 26 From young massive star cluster to old globular: the LV0 relationship as a diagnostic tool. DE GRIJS R., WILKINSON M.I. and TADHUNTER C.N.
2006A&A...448..881B 1 41 101 Dynamical mass estimates for two luminous star clusters in galactic merger remnants. BASTIAN N., SAGLIA R.P., GOUDFROOIJ P., et al.
2007MNRAS.382.1877M 75               F     1 50 22 Cluster and nebular properties of the central star-forming region of NGC 1140. MOLL S.L., MENGEL S., DE GRIJS R., et al.
2008A&A...489.1091M 75             C       1 35 28 Young star clusters in interacting galaxies - NGC 1487 and NGC 4038/4039. MENGEL S., LEHNERT M.D., THATTE N.A., et al.
2008AN....329..944M 23 0 Young star clusters in the Antennae galaxies and NGC 1487. MENGEL S., LEHNERT M.D., THATTE N., et al.
2009A&A...508L...5P 15       D               1 46 3 How universal are the two young cluster sequences?. The cases of the LMC, SMC, M 83, and the Antennae. PFALZNER S. and ECKART A.
2007ChJAA...7..155D 75             C       1 63 64 The Long-term Survival Chances of Young Massive Star Clusters. DE GRIJS R. and PARMENTIER G.
2011MNRAS.410L...6G 78               F     1 43 125 The distinction between star clusters and associations. GIELES M. and PORTEGIES ZWART S.F.
2010ARA&A..48..431P 94       D       C       2 167 902 Young massive star clusters. PORTEGIES ZWART S.F., McMILLAN S.L.W. and GIELES M.
2013MNRAS.436.2852B 16       D               1 130 81 Constraining globular cluster formation through studies of young massive clusters - I. A lack of ongoing star formation within young clusters. BASTIAN N., CABRERA-ZIRI I., DAVIES B., et al.
2017A&A...597A..28B 125 55 How can young massive clusters reach their present-day sizes? BANERJEE S. and KROUPA P.

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