| dc.contributor.author | Kobayashi, C | |
| dc.date.accessioned | 2014-01-15T15:30:32Z | |
| dc.date.available | 2014-01-15T15:30:32Z | |
| dc.date.issued | 2003-04 | |
| dc.identifier.citation | Kobayashi , C 2003 , ' The origin of elliptical galaxies inferred from their metallicity gradients ' , Astrophysics and Space Science , vol. 284 , no. 2 , pp. 853-856 . https://doi.org/10.1023/A:1024066522919 | |
| dc.identifier.issn | 0004-640X | |
| dc.identifier.other | PURE: 811359 | |
| dc.identifier.other | PURE UUID: 40e63b45-2b99-4a4a-befb-0d41c3ef31a0 | |
| dc.identifier.other | WOS: 000183320500111 | |
| dc.identifier.other | Scopus: 0346497597 | |
| dc.identifier.other | ORCID: /0000-0002-4343-0487/work/62750415 | |
| dc.identifier.uri | http://hdl.handle.net/2299/12539 | |
| dc.description.abstract | We simulate the chemodynamical evolution of elliptical galaxies using our GRAPE-SPH code. We succeed in reproducing the observed variety of the radial metallicity gradients, from which we discuss the origin of elliptical galaxies. | en |
| dc.format.extent | 4 | |
| dc.language.iso | eng | |
| dc.relation.ispartof | Astrophysics and Space Science | |
| dc.subject | EVOLUTION | |
| dc.title | The origin of elliptical galaxies inferred from their metallicity gradients | en |
| dc.contributor.institution | Centre for Astrophysics Research | |
| dc.contributor.institution | School of Physics, Engineering & Computer Science | |
| dc.contributor.institution | Department of Physics, Astronomy and Mathematics | |
| dc.description.status | Peer reviewed | |
| rioxxterms.versionofrecord | https://doi.org/10.1023/A:1024066522919 | |
| rioxxterms.type | Journal Article/Review | |
| herts.preservation.rarelyaccessed | true | |
