Browsing by Author "Ginsburg, Adam"

Now showing items 1-4 of 4

    • Cloud Structure of Three Galactic Infrared Dark Star-forming Regions from Combining Ground- and Space-based Bolometric Observations 

      Lin, Yuxin; Liu, Hauyu Baobab; Dale, James E.; Li, D.; Busquet, Gemma; Zhang, Zhi Yu; Ginsburg, Adam; Galván-Madrid, Roberto; Kovács, Attila; Koch, Eric; Qian, Lei; Wang, Ke; Longmore, Steve; Chen, Huei Ru; Walker, Daniel (2017-05-02)
      We have modified the iterative procedure introduced by Lin et al., to systematically combine the submillimeter images taken from ground-based (e.g., CSO, JCMT, APEX) and space (e.g., Herschel, Planck) telescopes. We applied ...

    • An Ionized Outflow in Orion-KL Source I? 

      Wright, Melvyn; Hirota, Tomoya; Forbrich, Jan; Plambeck, Richard; Bally, John; Goddi, Ciriaco; Ginsburg, Adam; McGuire, Brett (2023-03-01)
      We present images at 6 and 14 GHz of Source I (SrcI) in the Kleinmann–Low Nebula in Orion. At higher frequencies, from 43 to 340 GHz, images of this source are dominated by thermal emission from dust in a 100 au diameter ...

    • The Orion Protostellar Explosion and Runaway Stars Revisited : Stellar Masses, Disk Retention, and an Outflow from the Becklin-Neugebauer Object 

      Bally, John; Ginsburg, Adam; Forbrich, Jan; Vargas-Gonzalez, Jaime (2020-02-01)
      The proper motions of the three stars ejected from Orion's OMC1 cloud core are combined with the requirement that their center of mass is gravitationally bound to OMC1 to show that radio source I (Src I) is likely to have ...

    • 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 ...