tokens: Acknowledgements This paper is based on observations obtained at the Gemini Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the NSF on behalf of the Gemini partnership: the National Science Foundation (United States), the National Research Council (Canada), CONICYT (Chile), the Australian Research Council (Australia), Ministério da Ciência, Tecnologia e Inovação (Brazil) and Ministerio de Ciencia, Tecnología e Innovación Productiva (Argentina) and also on observations collected at the European Organisation for Astronomical Research in the Southern hemisphere under ESO programmes 079.C-0328(A) and 079.C-0328(B). This research has also made use of the NED, which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. Some of the data presented in this paper were based on observations made with the NASA/ESA HST, obtained from the data archive at the Space Telescope Institute. STScI is operated by the association of Universities for Research in Astronomy, Inc. under the NASA contract NAS 5-26555. This publication also makes use of data products from the Two Micron All Sky Survey, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation. TVRacknowledges CNPq for the financial support under the grant 304321/2016-8. JES acknowledges FAPESP for the financial support under the grant 2011/51680-6. DM acknowledges CNPq for the financial support under the grant 312987/2016-1. The optical data were obtained under grant support from Instituto do Milênio, MEGALIT (AGR). RBM acknowledges CAPES (Coordenação de Aperfeiçoamento de Pessoal de Nível Superior). Finally, we thank Roberto Cid Fernandes for carefully reading the manuscript, which improved a lot the quality of this work, and also Juliana Cristina Motter, for English revision. We also thank the anonymous referee for valuable insights that also enriched this paper.
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