Browsing by Author "cbd72b5e-898b-4ec0-b3eb-939505ea30c3"

Now showing items 1-4 of 4

    • ALMA observations of the Th 28 protostellar disk A new example of counter-rotation between disk and optical jet 
      Louvet, Fabien; Dougados, Catherine; Cabrit, S.; Hales, A.; Pinte, Christophe; Ménard, F.; Bacciotti, F.; Coffey, D.; Mardones Pérez, Diego; Bronfman Aguiló, Leonardo; Gueth, F. (EDP Sciences, 2016)
      Aims. Recently, differences in Doppler shifts across the base of four close classical T Tauri star jets have been detected with the HST in optical and near-ultraviolet (NUV) emission lines, and these Doppler shifts were ...
    • Flybys in protoplanetary discs – II. Observational signatures 
      Cuello, Nicolás; Louvet, Fabien; Mentiplay, Daniel; Pinte, Christophe; Price, Daniel J.; Winter, Andrew J.; Nealon, Rebecca; Menard, Francois; Lodato, Giuseppe; Dipierro, Giovanni; Christiaens, Valentín; Montesinos, Matías; Cuadra, Jorge; Laibe, Guillaume; Cieza, Lucas; Dong, Ruobing; Alexander, Richard (Oxford, 2020)
      Tidal encounters in star clusters perturb discs around young protostars. In Cuello et al., we detailed the dynamical signatures of a stellar flyby in both gas and dust. Flybys produce warped discs, spirals with evolving ...
    • Interferometric Mapping of Magnetic fields: The Alma view of the Massive star-forming clump W43-MM1 
      Cortes, Paulo; Girart, Josep; Hull, Charles; Sridharan, Tirupati; Louvet, Fabien; Plambeck, Richard; Li, Zhi-Yun; Crutcher, Richard; Lai, Shih-Ping (IOP, 2016)
      Here, we present the first results from ALMA observations of 1 mm polarized dust emission toward the W43-MM1 high-mass star-forming clump. We have detected a highly fragmented filament with source masses ranging from 14 ...
    • Tracing extended low-velocity shocks through SiO emission Case study of the W43-MM1 ridge 
      Louvet, Fabien; Motte, F.; Gusdorf, A.; Lu'o'ng, Q. Nguyen; Lesaffre, P.; Duarte Cabral, A.; Maury, A.; Schneider, N.; Hill, T.; Schilke, P.; Gueth, F. (EDP Sciences, 2016)
      Aims. Previous literature suggests that the densest structures in the interstellar medium form through colliding flows, but patent evidence of this process is still missing. Recent literature proposes using SiO line emission ...