| Texto completo | |
| Autor(es): |
Michtchenko, Tatiana A.
[1]
;
Lepine, Jacques R. D.
[1]
;
Perez-Villegas, Angeles
[1]
;
Vieira, Ronaldo S. S.
[1]
;
Barros, Douglas A.
[2]
Número total de Autores: 5
|
| Afiliação do(s) autor(es): | [1] Univ Sao Paulo, IAG, Rua Matao, 1226 Cidade Univ, BR-05508090 Sao Paulo - Brazil
[2] Rua Sessenta Tres 125, BR-53090393 Olinda, Pernambuco - Brazil
Número total de Afiliações: 2
|
| Tipo de documento: | Artigo Científico |
| Fonte: | Astrophysical Journal Letters; v. 863, n. 2 AUG 20 2018. |
| Citações Web of Science: | 4 |
| Resumo | |
The aim of this Letter is to contribute to the understanding of the stellar velocity distribution in the solar neighborhood (SN). We propose that the structures on the U-V planes, known as the moving groups, can be mainly explained by the spiral arms perturbations. The applied model of the Galactic disk and spiral arms, with the parameters defined by observational data and with pattern speed Omega(p) = 28.0 km s(-1) kpc(-1), is the same that allowed us to explain the origin of the Local Arm and the Sun's orbit trapped inside the corotation resonance (CR). We show that the U-V picture of the SN consists of the main component, associated with the CR, and the inner and outer structures, which we could associate with the Hercules and Sirius streams, respectively. The Coma-Berenices and Hyades-Pleiades groups, and the Sun itself, belong to the main part. The substructures of Hercules are formed mainly by the nearby 8/1, 12/1, and even 6/1 inner Lindblad resonances, while Sirius is shaped by the bulk of overlapping outer Lindblad resonances, -8/1, -12/1, -16/1, which are stuck to the CR. This richness in resonances only exists near corotation, which should be of the spiral arms, not of the Galactic bar, whose stable corotation zone is far away from the Sun. The model's predictions of the velocity distribution match qualitatively and quantitatively the distribution provided by Gaia data release 2. (AU) | |
| Processo FAPESP: | 15/10577-9 - Caos e integrabilidade em discos galácticos |
| Beneficiário: | Ronaldo Savioli Sumé Vieira |
| Linha de fomento: | Bolsas no Brasil - Pós-Doutorado |
| Processo FAPESP: | 09/54006-4 - Um cluster de computadores para o Departamento de Astronomia do IAG-USP e para o Núcleo de Astrofísica da UNICSUL |
| Beneficiário: | Elisabete Maria de Gouveia Dal Pino |
| Linha de fomento: | Auxílio à Pesquisa - Programa Equipamentos Multiusuários |
| Processo FAPESP: | 17/15893-1 - Órbitas de aglomerados globulares do bojo: formação e evolução da Via Láctea |
| Beneficiário: | Maria de Los Angeles Perez Villegas |
| Linha de fomento: | Bolsas no Brasil - Pós-Doutorado |