Now showing items 1-3 of 3

    • 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 ...
    • Prisinzano, L.; Damiani, F.; Kalari, V.; Jeffries, R.; Bonito, R.; Micela, G.; Wright, N. J.; Jackson, R. J.; Tognelli, E.; Guarcello, M. G.; Vink, J. S.; Klutsch, A.; Jiménez-Esteban, F. M.; Roccatagliata, V.; Tautvaišiene, G.; Gilmore, G.; Randich, S.; Alfaro, E. J.; Fla (EDP Sciences, 2019)
      Context. In very young clusters, stellar age distribution is empirical proof of the duration of star cluster formation and thus it gives indications of the physical mechanisms involved in the star formation process. ...
    • Wright, Nicholas J.; Jeffries, R. D.; Jackson, R. J.; Bayo, A.; Bonito, R.; Damiani, F.; Kalari, V.; Lanzafame, A. C.; Pancino, E.; Parker, R. J.; Prisinzano, L.; Randich, S.; Vink, J. S.; Alfaro, E. J.; Bergemann, M.; Franciosini, E.; Gilmore, G.; Gonneau, A.; Hourihane, (Oxford University Press, 2019)
      The combination of precise radial velocities from multi-object spectroscopy and highly accurate proper motions from Gaia DR2 opens up the possibility for detailed 3D kinematic studies of young star-forming regions and ...