Browsing by Author "48afcf47-be09-4f5d-921b-154dd25a6e46"

Now showing items 1-2 of 2

    • ALMA survey of massive cluster progenitors from ATLASGAL: Limited fragmentation at the early evolutionary ... 
      Csengeri, T.; Bontemps, S.; Wyrowski, F.; Motte, F.; Menten, K. M.; Beuther, H.; Bronfman Aguiló, Leonardo; Commerçon, B.; Chapillón, E.; Duarte Cabral, A.; Fuller, G. A.; Henning, Th; Leurini, S.; Longmore, S.; Palau, A.; Peretto, N.; Schuller, F.; Tan, J. C.; Testi, L.; Traficante, A.; Urquhart, J. S. (EDP Sciences, 2017)
      The early evolution of massive cluster progenitors is poorly understood. We investigate the fragmentation properties from 0.3 pc to 0.06 pc scalesof a homogenous sample of infrared-quiet massive clumps within 4.5 kpc ...
    • The Hi-GAL catalogue of dusty filamentary structures in the Galactic plane 
      Schisano, Eugenio; Molinari, S.; Elia, D.; Benedettini, M.; Olmi, L.; Pezzuto, S.; Traficante, A.; Brescia, M.; Cavuoti, S.; Di Giorgio, A. M.; Liu, S. J.; Moore, T. J. T.; Noriega Crespo, A.; Riccio, G.; Baldeschi, A.; Becciani, U.; Peretto, N.; Merello, M.; Vitello, F.; Zavagno, A.; Beltrán, M. T.; Cambrésy, L.; Eden, D. J.; Causi, G. Li; Molinaro, M.; Palmeirim, P.; Sciacca, E.; Testi, L.; Umana, G.; Whitworth, A. P. (Oxford University Press, 2020)
      The recent data collected by Herschel have confirmed that interstellar structures with a filamentary shape are ubiquitously present in the Milky Way. Filaments are thought to he formed by several physical mechanisms acting ...