Now showing items 1-2 of 2

    • Thermal Feedback in the High-mass Star- and Cluster-forming Region W51 

      Ginsburg, Adam; Goddi, Ciriaco; Kruijssen, J. M.Diederik; Bally, John; Smith, Rowan; Galván-Madrid, Roberto; Mills, Elisabeth A.C.; Wang, Ke; Dale, James E.; Darling, Jeremy; Rosolowsky, Erik; Loughnane, Robert; Testi, Leonardo; Bastian, Nate (2017-06-16)
      High-mass stars have generally been assumed to accrete most of their mass while already contracted onto the main sequence, but this hypothesis has not been observationally tested. We present ALMA observations of a 3 × 1.5 ...
    • Which feedback mechanisms dominate in the high-pressure environment of the Central Molecular Zone? 

      Barnes, Ashley T; Longmore, Steven N; Dale, James; Krumholz, Mark R.; Kruijssen, J. M.Diederik; Bigiel, Frank (2020-09-08)
      Supernovae (SNe) dominate the energy and momentum budget of stellar feedback, but the efficiency with which they couple to the interstellar medium (ISM) depends strongly on how effectively early, pre-SN feedback clears ...