| dc.date.accessioned | 2020-03-11T20:37:10Z | |
| dc.date.accessioned | 2022-10-18T23:05:31Z | |
| dc.date.available | 2020-03-11T20:37:10Z | |
| dc.date.available | 2022-10-18T23:05:31Z | |
| dc.date.created | 2020-03-11T20:37:10Z | |
| dc.date.issued | 2008 | |
| dc.identifier | http://hdl.handle.net/10533/241230 | |
| dc.identifier | 15010003 | |
| dc.identifier | WOS:000258808300035 | |
| dc.identifier | no scielo | |
| dc.identifier | eid=2-s2.0-48049113954 | |
| dc.identifier.uri | https://repositorioslatinoamericanos.uchile.cl/handle/2250/4472569 | |
| dc.description.abstract | We determine the underlying shapes of spiral and elliptical galaxies in the Sloan Digital Sky Survey Data Release 6 from the observed distribution of projected galaxy shapes, taking into account the effects of dust extinction and reddening. We assume that | |
| dc.language | eng | |
| dc.relation | https://doi.org/10.1111/j.1365-2966.2008.13480.x | |
| dc.relation | 10.1111/j.1365-2966.2008.13480.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 shapes of galaxies in the Sloan Digital Sky Survey | |
| dc.type | Articulo | |
