dc.date.accessioned | 2020-03-11T20:25:39Z | |
dc.date.accessioned | 2022-10-18T22:39:37Z | |
dc.date.available | 2020-03-11T20:25:39Z | |
dc.date.available | 2022-10-18T22:39:37Z | |
dc.date.created | 2020-03-11T20:25:39Z | |
dc.date.issued | 2008 | |
dc.identifier | http://hdl.handle.net/10533/237849 | |
dc.identifier | 15010003 | |
dc.identifier | WOS:000258652200019 | |
dc.identifier | no scielo | |
dc.identifier | eid=2-s2.0-49749084716 | |
dc.identifier.uri | https://repositorioslatinoamericanos.uchile.cl/handle/2250/4469188 | |
dc.description.abstract | Recent near- and mid-infrared surveys have brought evidence that the Milky Way continues to form massive clusters. We carry out a program to determine the basic physical properties of the new massive cluster candidate [DBS2003]179. Medium-resolution K-ban | |
dc.language | eng | |
dc.relation | https://doi.org/10.1051/0004-6361:20079255 | |
dc.relation | 10.1051/0004-6361:20079255 | |
dc.rights | info:eu-repo/semantics/openAccess | |
dc.rights | Atribución-NoComercial-SinDerivadas 3.0 Chile | |
dc.rights | http://creativecommons.org/licenses/by-nc-nd/3.0/cl/ | |
dc.title | The young Galactic star cluster [DBS2003] 179 | |
dc.type | Articulo | |