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[L99] n5236-502 , the SIMBAD biblio (12 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST01:40:14 |
Bibcode/DOI | Score |
in Title|Abstract| Keywords |
in a table | in teXt, Caption, ... | Nb occurence | Nb objects in ref |
Citations (from ADS) |
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 LV-σ0 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. |