The transition between star clusters and dwarf galaxies. On the existence of a mass-radius relation for star clusters of masses > 10-7 Mo: are these objects formed in mergers of stellar systems?

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dc.contributor.authorKissler-Patig, M.
dc.contributor.authorJordán Colzani, Andrés Cristóbal
dc.date.accessioned2017-04-11T20:51:10Z
dc.date.available2017-04-11T20:51:10Z
dc.date.issued2006
dc.identifier.doi10.1051/0004-6361:20054384
dc.identifier.issn0935-4956
dc.identifier.urihttps://doi.org/10.1051/0004-6361:20054384
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/18891
dc.language.isoen
dc.nota.accesocontenido completo
dc.relation.isformatofAstronomy and Astrophysics Review. Vol. 448, no. 3 (2006), p. [1031]-1035
dc.revistaAstronomy and Astrophysics Reviewes_ES
dc.rightsacceso abierto
dc.subject.ddc520
dc.subject.deweyAstronomíaes_ES
dc.subject.otherEstrellas - Cúmuloses_ES
dc.subject.otherCúmulos de Galaxiases_ES
dc.subject.otherGalaxias enanases_ES
dc.subject.otherFotometría astronómicaes_ES
dc.titleThe transition between star clusters and dwarf galaxies. On the existence of a mass-radius relation for star clusters of masses > 10-7 Mo: are these objects formed in mergers of stellar systems?es_ES
dc.typeartículo
dc.volumenVol. 448
sipa.codpersvinculados176960
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