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    • 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 ...
    • Mesa, D.; Bonnefoy, M.; Gratton, R.; Van Der Plas, G.; D'Orazi, V.; Sissa, E.; Zurlo, A.; Rigliaco, E.; Schmidt, T.; Langlois, M.; Vigan, A.; Ubeira Gabellini, M. G.; Desidera, S.; Antoniucci, S.; Barbieri, M.; Benisty, Myriam; Boccaletti, A.; Claudi, R.; Fedele, D.; Gasparri, (EDP Sciences, 2019)
      Aims. R Coronae Australis (R CrA) is the brightest star of the Coronet nebula of the Corona Australis (CrA) star forming region. This star is very red in color, probably due to dust absorption, and is strongly variable. ...