Browsing by Author "b7cfbfcf-8d74-4cb9-9a2b-57c2ec6ed44e"

Now showing items 1-5 of 5

    • A tale of three cities OmegaCAM discovers multiple sequences in the color magnitude diagram of the Orion ... 
      Beccari, G.; Petr Gotzens, M. G.; Boffin, H. M. J.; Romaniello, M.; Fedele, D.; Carraro, Giovanni; De Marchi, G.; de Wit, W. J.; Drew, J. E.; Kalari, V. M.; Manara, C. F.; Martin, E. L.; Mieske, S.; Panagia, N.; Testi, L.; Vink, J. S.; Walsh, J. R.; Wright, N. J. (EDP Sciences, 2017)
      As part of the accretion discs in H alpha with OmegaCAM (ADHOC) survey, we imaged a region of 12x8 square degrees around the Orion Nebula Cluster in r, i and H alpha. Thanks to the high-quality photometry obtained, we ...
    • On the assessment of the nature of open star clusters and the determination of their basic parameters with ... 
      Carraro, Giovanni; Baume, Gustavo; Seleznev, Anton F.; Costa Hechenleitner, Edgardo (Springer, 2017)
      Our knowledge of stellar evolution and of the structure and chemical evolution of the Galactic disk largely builds on the study of open star clusters. Because of their crucial role in these relevant topics, large ...
    • Stellar populations in the Carina region The Galactic plane at l=291 degrees 
      Molina-Lera, J.; Baume, G.; Gamen, R.; Costa Hechenleitner, Edgardo; Carraro, Giovanni (EDP Sciences, 2016-08)
      Context. Previous studies of the Carina region have revealed its complexity and richness as well as a significant number of early-type stars. However, in many cases, these studies only concentrated on the central region ...
    • The magellanic bridge cluster NGC 796: deep optical AO imaging reveals the stellar content and initial mass ... 
      Kalari, Venu M.; Carraro, Giovanni; Evans, Christopher J.; Rubio López, Mónica (IOP Publishing Ltd, 2018)
      NGC 796 is a massive young cluster located 59 kpc from us in the diffuse intergalactic medium of the 1/5-1/10 Z(circle dot) Magellanic Bridge, allowing us to probe variations in star formation and stellar evolution processes ...
    • VVV DR1: The first data release of the Milky Way bulge and southern plane from the near-infrared ESO public ... 
      Saito, R. K.; Hempel, M.; Minniti, D.; Lucas, P. W.; Rejkuba, M.; Toledo, I.; Gonzalez, O. A.; Alonso-García, J.; Irwin, M.; Gonzalez-Solares, E.; Hodgkin, S. T.; Lewis, J. R.; Cross, N.; Ivanov, V. D.; Kerins, E.; Emerson, J. P.; Soto, M.; Amôres, E. B.; Gurovich, S.; Dékány, I.; Angeloni, R.; Beamin, J. C.; Catelan, M.; Padilla, N.; Zoccali, M.; Pietrukowicz, P.; Moni Bidin, C.; Mauro, F.; Geisler, D.; Folkes, S. L.; Sale, S. E.; Borissova, J.; Kurtev, R.; Ahumada, A. V.; Alonso, M. V.; Adamson, A.; Arias, J. I.; Bandyopadhyay, R. M.; Barbá, R. H.; Barbuy, B.; Baume, G. L.; Bedin, L. R.; Bellini, A.; Benjamin, R.; Bica, E.; Bonatto, C.; Bronfman Aguiló, Leonardo; Carraro, Giovanni; Chenè, A. N.; Clariá, J. J.; Clarke, J. R. A.; Contreras, C.; Corvillón, A.; Grijs, R. de; Dias, B.; Drew, J. E.; Fariña, C.; Feinstein, C.; Fernández Lajús, E.; Gamen, R.; Gieren, W.; Goldman, B.; González-Fernández, C.; Grand, R. J. J.; Gunthardt, G.; Hambly, N. C.; Hanson, M. M.; Helminiak, K. G.; Hoare, M. G.; Huckvale, L.; Jordán, A.; Kinemuch, K.; Longmore, A.; López Corredoira, M.; Maccarone, T.; Majaess, D.; Martín, E. L.; Masetti, N.; Mennickent, R. E.; Mirabel, I. F.; Monaco, L.; Morelli, L.; Motta, V.; Palma, T.; Parisi, M. C.; Parker, Q.; Peñaloza, F.; Pietrzynski, G.; Pignata Libralato, Giuliano; Popescu, B.; Read, M. A.; Rojas, A.; Roman-Lopes, A.; Ruiz González, María Teresa; Saviane, I.; Schreiber, M. R.; Schröder, A. C.; Sharma, S.; Smith, M. D.; Sodré Jr., L.; Stead, J.; Stephens, A. W.; Tamura, M.; Tappert, C.; Thompson, M. A.; Valenti, E.; Vanzi, L.; Walton, N. A.; Weidmann, W.; Zijlstr, A. (2012-01)
      Context. The ESO public survey VISTA variables in the Vía Láctea (VVV) started in 2010. VVV targets 562 sq. deg in the Galactic bulge and an adjacent plane region and is expected to run for about five years. Aims. We ...