| dc.date.accessioned | 2020-03-11T20:29:44Z | |
| dc.date.accessioned | 2022-10-18T22:47:29Z | |
| dc.date.available | 2020-03-11T20:29:44Z | |
| dc.date.available | 2022-10-18T22:47:29Z | |
| dc.date.created | 2020-03-11T20:29:44Z | |
| dc.date.issued | 2009 | |
| dc.identifier | http://hdl.handle.net/10533/238892 | |
| dc.identifier | 15010003 | |
| dc.identifier | WOS:000266549600044 | |
| dc.identifier | no scielo | |
| dc.identifier | eid=2-s2.0-67651133232 | |
| dc.identifier.uri | https://repositorioslatinoamericanos.uchile.cl/handle/2250/4470231 | |
| dc.description.abstract | In this paper, we study the variations of group galaxy properties according to the assembly history in SDSS-DR6 selected groups. Using mock SDSS group catalogues, we find two suitable indicators of group formation time: i) the isolation of the group, defi | |
| dc.language | eng | |
| dc.relation | https://doi.org/10.1111/j.1365-2966.2009.14491.x | |
| dc.relation | 10.1111/j.1365-2966.2009.14491.x | |
| 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 influence of halo assembly on galaxies and galaxy groups | |
| dc.type | Articulo | |
