| dc.contributor.author | Kobayashi, C. | |
| dc.contributor.author | Nakasato, N. | |
| dc.contributor.author | Nomoto, K. | |
| dc.contributor.editor | Makino, J. | |
| dc.contributor.editor | Hut, P. | |
| dc.date.accessioned | 2015-01-13T14:32:38Z | |
| dc.date.available | 2015-01-13T14:32:38Z | |
| dc.date.issued | 2003 | |
| dc.identifier.citation | Kobayashi , C , Nakasato , N & Nomoto , K 2003 , Chemodynamical evolution of the Milky Way . in J Makino & P Hut (eds) , Astrophysical Supercomputing Using Particle Simulations . Astronomical Society of the Pacific , SAN FRANCISCO , pp. 419-420 , 208th Symposium of the International Astronomical Union , Tokyo , Japan , 10/07/01 . | |
| dc.identifier.citation | conference | |
| dc.identifier.isbn | 1-58381-139-7 | |
| dc.identifier.other | PURE: 811303 | |
| dc.identifier.other | PURE UUID: 099c52b5-a9ab-495a-a098-9bda7ed724de | |
| dc.identifier.other | WOS: 000183793400060 | |
| dc.identifier.other | ORCID: /0000-0002-4343-0487/work/62750428 | |
| dc.identifier.uri | http://hdl.handle.net/2299/15191 | |
| dc.description.abstract | We simulate the chemodynamical evolution of the Milky Way using our GRAPE-SPH code, and reproduce the age-metallicity relation, the [O/Fe]-[Fe/H] relation, and the metallicity distribution. | en |
| dc.format.extent | 2 | |
| dc.language.iso | eng | |
| dc.publisher | Astronomical Society of the Pacific | |
| dc.relation.ispartof | Astrophysical Supercomputing Using Particle Simulations | |
| dc.title | Chemodynamical evolution of the Milky Way | 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 | |
| rioxxterms.type | Other | |
| herts.preservation.rarelyaccessed | true | |
