Gemini GMOS IFU Study of BAL QSOs: Decoupling the BAL QSO, Starburst, NLR and Supergiant Bubbles
Lipari, S.; Sanchez, S. F.; Bergmann, M.;Terlevich, R.; Punsly, B.; Mediavilla, E.;Dottori, H.; Taniguchi, Y.; Ajiki, M.; García, B.;Zheng, W.; Acosta, J.; Jahnke, J.. Gemini GMOS IFU Study of BAL QSOs: Decoupling the BAL QSO, Starburst, NLR and Supergiant Bubbles. Boletín de la Asociación Argentina de Astronomía. 2006, Vol. vol.49, p.267-270, p. -2006.
= 200 pc). The physical properties of the 4 expanding nuclear bubbles (in Mrk 231) and the NLR were analysed. Finally, the composite hyper-wind scenario is suggested for the origin of BALs and giant Ly-alpha blobs. The importance of study the end phase of BAL+IR QSOs, and ellipticals (i.e. galaxy remnants) is discussed.
= 200 pc). The physical properties of the 4 expanding nuclear bubbles (in Mrk 231) and the NLR were analysed. Finally, the composite hyper-wind scenario is suggested for the origin of BALs and giant Ly-alpha blobs. The importance of study the end phase of BAL+IR QSOs, and ellipticals (i.e. galaxy remnants) is discussed.