| 1. Identificação | |
| Tipo de Referência | Artigo em Revista Científica (Journal Article) |
| Site | mtc-m21b.sid.inpe.br |
| Código do Detentor | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
| Identificador | 8JMKD3MGP5W34M/3FA7RGQ |
| Repositório | sid.inpe.br/mtc-m21b/2013/11.27.13.23.10 |
| Última Atualização | 2014:01.20.15.44.22 (UTC) administrator |
| Repositório de Metadados | sid.inpe.br/mtc-m21b/2013/11.27.13.23.11 |
| Última Atualização dos Metadados | 2018:06.04.03.14.16 (UTC) administrator |
| DOI | 10.1093/mnras/stt884 |
| ISSN | 0035-8711 |
| Rótulo | isi 2013-11 |
| Chave de Citação | CarrubaDoNeRoHuSo:2013:MuApAs |
| Título | A multidomain approach to asteroid families' identification  |
| Ano | 2013 |
| Mês | Aug. |
| Data de Acesso | 19 abr. 2024 |
| Tipo Secundário | PRE PI |
| Número de Arquivos | 1 |
| Tamanho | 3643 KiB |
| 2. Contextualização | |
| Autor | 1 Carruba, V. 2 Domingos, Rita de Cássia 3 Nesvorny, D. 4 Roig, F. 5 Huaman, M. E. 6 Souami, D. |
| Grupo | 1 2 ETE-ETE-INPE-MCTI-GOV-BR |
| Afiliação | 1 Univ Estadual Paulista, UNESP, Grp Dinam Orbital & Planetol, BR-12516410 Guaratingueta, SP, Brazil. 2 Instituto Nacional de Pesquisas Espaciais (INPE) 3 SWRI, Boulder, CO 80302 USA. 4 ON, BR-20921400 Rio De Janeiro, RJ, Brazil. 5 Univ Estadual Paulista, UNESP, Grp Dinam Orbital & Planetol, BR-12516410 Guaratingueta, SP, Brazil. 6 Univ Paris 06, F-75005 Paris, France.; UPMC, Observ Paris, SYRTE, CNRS UMR 8630, F-75014 Paris, France. |
| Endereço de e-Mail | marcelo.pazos@inpe.br |
| Revista | Monthly Notices of the Royal Astronomical Society |
| Volume | 433 |
| Número | 3 |
| Páginas | 2075-2096 |
| Nota Secundária | A1 A1 A1 A2 A2 A2 B3 C |
| Histórico (UTC) | 2018-06-04 03:14:16 :: administrator -> marcelo.pazos@inpe.br :: 2013 |
| 3. Conteúdo e estrutura | |
| É a matriz ou uma cópia? | é a matriz |
| Estágio do Conteúdo | concluido |
| Transferível | 1 |
| Tipo do Conteúdo | External Contribution |
| Tipo de Versão | finaldraft |
| Palavras-Chave | Celestial mechanics minor planets asteroids: general |
| Resumo | It has been shown that large families are not limited to what found by hierarchical clustering methods in the domain of proper elements (a, e, sin(i)), which seems to be biased to find compact, relatively young clusters, but that there exists an extended population of objects with similar taxonomy and geometric albedo, which can extend to much larger regions in proper elements and frequencies domains: the family `halo'. Numerical simulations can be used to provide estimates of the age of the family halo, which can then be compared with ages of the family obtained with other methods. Determining a good estimate of the possible orbital extension of a family halo is therefore quite important, if one is interested in determining its age and, possibly, the original ejection velocity field. Previous works have identified families' haloes by an analysis in proper elements domains, or by using Sloan Digital Sky Survey-Moving Object Catalog data, fourth release (SDSS-MOC4) multiband photometry to infer the asteroid taxonomy, or by a combination of the two methods. The limited number of asteroids for which geometric albedo was known until recently discouraged in the past the extensive use of this additional parameter, which is however of great importance in identifying an asteroid taxonomy. The new availability of geometric albedo data from the Wide-field Infrared Survey Explorer (WISE) mission for about 100 000 asteroids significantly increased the sample of objects for which such information, with some errors, is now known. In this work, we proposed a new method to identify families' haloes in a multidomain space composed by proper elements, SDSS-MOC4 (a*, i - z) colours, and WISE geometric albedo for the whole main belt (and the Hungaria and Cybele orbital regions). Assuming that most families were created by the breakup of an undifferentiated parent body, they are expected to be homogeneous in colours and albedo. The new method is quite effective in determining objects belonging to a family halo, with low percentages of likely interlopers, and results that are quite consistent in term of taxonomy and geometric albedo of the halo members. |
| Área | ETES |
| Arranjo | urlib.net > Fonds > Produção anterior à 2021 > CGETE > A multidomain approach... |
| Conteúdo da Pasta doc | acessar |
| Conteúdo da Pasta source | não têm arquivos |
| Conteúdo da Pasta agreement | não têm arquivos |
| 4. Condições de acesso e uso | |
| URL dos dados | http://urlib.net/ibi/8JMKD3MGP5W34M/3FA7RGQ |
| URL dos dados zipados | http://urlib.net/zip/8JMKD3MGP5W34M/3FA7RGQ |
| Idioma | en |
| Grupo de Usuários | administrator marcelo.pazos@inpe.br |
| Grupo de Leitores | administrator marcelo.pazos@inpe.br |
| Visibilidade | shown |
| Política de Arquivamento | allowpublisher allowfinaldraft |
| Permissão de Leitura | allow from all |
| Permissão de Atualização | não transferida |
| 5. Fontes relacionadas | |
| Repositório Espelho | iconet.com.br/banon/2006/11.26.21.31 |
| Unidades Imediatamente Superiores | 8JMKD3MGPCW/3EUUDJE |
| Lista de Itens Citando | sid.inpe.br/bibdigital/2013/10.07.21.11 1 |
| Divulgação | WEBSCI; PORTALCAPES; COMPENDEX; SCOPUS. |
| Acervo Hospedeiro | sid.inpe.br/mtc-m21b/2013/09.26.14.25.20 |
| 6. Notas | |
| Campos Vazios | alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel electronicmailaddress format isbn lineage mark nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project resumeid rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject targetfile tertiarymark tertiarytype typeofwork url |
| 7. Controle da descrição | |
| e-Mail (login) | marcelo.pazos@inpe.br |
| atualizar | |
