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| NAME Serpens SVS 2 Cluster , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST23:20:47 |
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| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2003ARA&A..41...57L | 5 | 148 | 2488 | Embedded clusters in molecular clouds. | LADA C.J. and LADA E.A. | ||||
2004A&A...421..623K 
|
166 | 77 | The young stellar population in the Serpens Cloud Core: An ISOCAM survey. | KAAS A.A., OLOFSSON G., BONTEMPS S., et al. | |||||
| 2006MNRAS.365.1333W | 5 | 24 | 285 | The maximum stellar mass, star-cluster formation and composite stellar populations. | WEIDNER C. and KROUPA P. | ||||
|
2007PASJ...59.1185S
|
15 | D | 1597 | 41 | Water maser and ammonia survey toward IRAS sources in the Galaxy. I. H2O maser data. | SUNADA K., NAKAZATO T., IKEDA N., et al. | |||
| 2008ApJ...689..816S | 38 | X | 1 | 16 | 20 | The scale-free character of the cluster mass function and the universality of the stellar initial mass function. | SELMAN F.J. and MELNICK J. | ||
| 2009ApJ...705..468H | 205 | D | X | 6 | 29 | 34 | A mapping survey of dense clumps associated with embedded clusters: evolutionary stages of cluster-forming clumps. | HIGUCHI A.E., KURONO Y., SAITO M., et al. | |
| 2010MNRAS.401..275W | 15 | D | 1 | 173 | 198 | The relation between the most-massive star and its parental star cluster mass. | WEIDNER C., KROUPA P. and BONNELL I.A.D. | ||
| 2010ApJ...719.1813H | 435 | D | X C | 11 | 22 | 26 | A mapping survey of dense clumps associated with embedded clusters. II. Can clump-clump collisions induce stellar clusters? | HIGUCHI A.E., KURONO Y., SAITO M., et al. | |
|
2010A&A...519A..27D
|
39 | X | 1 | 13 | 29 | The physical and dynamical structure of Serpens. Two very different sub-(proto)clusters. | DUARTE-CABRAL A., FULLER G.A., PERETTO N., et al. | ||
| 2014ApJ...780...27P | 16 | D | 1 | 137 | 9 | The range of variation of the mass of the most massive star in stellar clusters derived from 35 million Monte Carlo simulations. | POPESCU B. and HANSON M.M. |
