Browsing by Author "Bally, J."

Now showing items 1-4 of 4

    • ALMA-IMF III. Investigating the origin of stellar masses: top-heavy core mass function in the W43-MM2&MM3 ... 
      Pouteau, Y.; Motte, F.; Nony, T.; Galván Madrid, R.; Men’shchikov, A.; Bontemps, S.; Robitaille, J. F.; Louvet, Fabien; Ginsburg, A.; López Sepulcre, A.; Dell’Ova, P.; Gusdorf, A.; Sanhueza, P.; Stutz, Amelia Marie; Brouillet, N.; Thomasson, B.; Armante, M.; Baug, T.; Bonfand, M.; Busquet, G.; Csengeri, T.; Cunningham, N.; Fernández López, M.; Liu, H. L.; Olguin, F.; Towner, A. P. M.; Bally, J.; Braine, J.; Bronfman Aguiló, Leonardo Jaime; González, M.; Hennebelle, P.; Lu, X.; Menten, K. M.; Moraux, E.; Tatematsu, K.; Walker, D.; Whitworth, A. P. (EDP Sciences, 2021)
      Aims. The processes that determine the stellar initial mass function (IMF) and its origin are critical unsolved problems, with profound implications for many areas of astrophysics. The W43-MM2&MM3 mini-starburst ridge ...
    • A cluster in the making: ALMA reveals the initial conditions for high-mass cluster formation 
      Rathborne, Jill; Longmore, S. N.; Jackson, J. M.; Alves, J. F.; Bally, J.; Bastian, N.; Contreras, Y.; Foster, J. B.; Garay Brignardello, Guido; Kruijssen, J. M.; Testi, L.; Walsh, A. J. (IOP PUBLISHING LTD, 2015)
      G0.253+0.016 is a molecular clump that appears to be on the verge of forming a high-mass cluster: its extremely low dust temperature, high mass, and high density, combined with its lack of prevalent star formation, make ...
    • A cluster in the making: alma reveals the initial conditions for high-mass cluster formation. 
      Rathborne, Jill; Longmore, S. N.; Jackson, J. M.; Alves, J. F.; Bally, J.; Bastian, N.; Contreras, Y.; Foster, J. B.; Garay Brignardello, Guido; Kruijssen, J. M. D.; Testi, L.; Walsh, A. J. (2015-04-01)
      G0.253+0.016 is a molecular clump that appears to be on the verge of forming a high-mass cluster: its extremely low dust temperature, high mass, and high density, combined with its lack of prevalent star formation, make ...
    • G0.253+0.016: A centrally condensed, high-mass protocluster. 
      Rathborne, Jill; Longmore, S. N.; Jackson, J. M.; Foster, J. B.; Contreras, Y.; Garay Brignardello, Guido; Testi, L.; Alves, J. F.; Bally, J.; Bastian, N.; Kruijssen, J. M. D.; Bressert, E. (The American Astronomical Society., 2014-04-25)
      Despite their importance as stellar nurseries and the building blocks of galaxies, very little is known about the formation of the highest mass clusters. The dense clump G0.253+0.016 represents an example of a clump that ...