On the possible generation of the young massive open clusters Stephenson 2 and BDSB122 by ω Centauri

• Autor(a) principal: Salerno, Gustavo Malta
• Data de Publicação: 2009
• Outros Autores: Bica, Eduardo Luiz Damiani, Bonatto, Charles Jose, Rodrigues, Irapuan
• Tipo de documento: Artigo
• Idioma: eng
• Título da fonte: Repositório Institucional da UFRGS
• Texto Completo: http://hdl.handle.net/10183/99255
• topic: Aglomerados estelares globulares; Formacao de estrelas; Galaxia; Gravitacao; Galaxy: globular clusters: individual: ωCentauri; Galaxy: open clusters and associations: individual: BDSB; Galaxy: open clusters and associations: individual: Stephenson 2

Context. Passing through the disk of a galaxy, a massive object such as a globular cluster can trigger star formation. Aims. We test the hypothesis that the most massive globular cluster in the Galaxy, ωCentauri, which crossed the disk approximately 24 ± 2Myr ago, may have triggered the formation of the open clusters Stephenson 2 and BDSB122. Methods. The orbits of ωCentauri, Stephenson 2, and BDSB122 are computed for the three-component model of Johnston, Hernquist & Bolte, which considers the disk, spheroidal, and halo gravitational potentials. Results. With the reconstructed orbit of ωCentauri, we show that the latest impact site is consistent, within significant uncertainties, with the birth-site of the young massive open clusters BDSB122 and Stephenson 2.Within the uncertainties, this scenario is consistent with the timescale of their backward motion in the disk, shock propagation and delayed star formation. Conclusions. Together with open cluster formation associated with density waves in spiral arms, the present results are consistent with massive globular clusters being additional progenitors of open clusters, the most massive ones in particular.