Recent Submissions

  • Complex Organic Molecules tracing shocks along the outflow cavity in the high-mass protostar IRAS 20126+4104 

    Palau, A; Walsh, C; Sánchez-Monge, Á; Girart, JM; Cesaroni, R; Jiménez-Serra, I; Fuente, A; Zapata, LA; Neri, R (Oxford University Press, 2017-01)
    We report on subarcsecond observations of complex organic molecules (COMs) in the high-mass protostar IRAS 20126+4104 with the Plateau de Bure Interferometer in its most extended configurations. In addition to the simple ...
  • Giant Planet Formation and Migration 

    Paardekooper, SJ; Johansen, A (Springer, 2018-01)
    Planets form in circumstellar discs around young stars. Starting with sub-micron sized dust particles, giant planet formation is all about growing 14 orders of magnitude in size. It has become increasingly clear over the ...
  • How does the cosmic large-scale structure bias the Hubble diagram? 

    Fleury, P; Clarkson, C; Maartens, R (IOP Publishing, 2017-03)
    The Hubble diagram is one of the cornerstones of observational cosmology. It is usually analysed assuming that, on average, the underlying relation between magnitude and redshift matches the prediction of a Friedmann-Lem ...
  • Dynamics of co in amorphous water-ice environments 

    Karssemeijer, LJ; Ioppolo, S; Van Hemert, MC; Van Der Avoird, A; Allodi, MA; Blake, GA; Cuppen, HM (IOP Publishing, 2013-12-30)
    The long-timescale behavior of adsorbed carbon monoxide on the surface of amorphous water ice is studied under dense cloud conditions by means of off-lattice, on-the-fly, kinetic Monte Carlo simulations. It is found that ...
  • Radiation Hydrodynamical Turbulence in Protoplanetary Disks: Numerical Models and Observational Constraints 

    Flock, M; NELSON, RP; Turner, NJ; Bertrang, GH-M; Carrasco-Gonzalez, C; Henning, T; Lyra, W; Teague, R (American Astronomical Society, 2017-11-27)
    Planets are born in protostellar disks, which are now observed with enough resolution to address questions about internal gas flows. Magnetic forces are possibly drivers of the flows, but ionization state estimates suggest ...
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