Showing 1–20 of 20 results
/ Date/ Name
Mar 14, 2014Coreshine in L1506C - Evidence for a primitive big-grain component or indication for a turbulent core history?Feb 7, 2014Detecting scattered light from low-mass molecular cores at 3.6 $μ$m - Impact of global effects on the observation of coreshineMay 11, 2010Dust-temperature of an isolated star-forming cloud: Herschel observations of the Bok globule CB244Aug 22, 2012The Earliest Phases of Star formation observed with Herschel (EPoS): The dust temperature and density distributions of B68Oct 26, 20043D Continuum radiative transfer in complex dust configurations around young stellar objects and active nuclei II. 3D Structure of the dense molecular cloud core Rho Oph DMay 11, 2010From high-mass starless cores to high-mass protostellar objectsFeb 15, 2004The 2D Continuum Radiative Transfer Problem: Benchmark Results for Disk ConfigurationsAug 31, 2007Zooming into the large circumstellar disk in M 17Jul 22, 2014A common column density threshold for scattering at 3.6 mum and water-ice in molecular cloudsOct 12, 2004Three-dimensional Continuum Radiative Transfer Images of a Molecular Cloud Core EvolutionMay 11, 2010The structured environments of embedded star-forming cores. PACS and SPIRE mapping of the enigmatic outflow source UYSO 1Oct 26, 2013Scattering from dust in molecular clouds: Constraining the dust grain size distribution through near-infrared cloudshine and infrared coreshineJan 10, 2008Probing the centre of the large circumstellar disc in M17Aug 17, 2015Grain size limits derived from 3.6 μm and 4.5 μm coreshineDec 1, 2009Direct evidence of dust growth in L183 from MIR light scatteringMar 17, 2006Ray-tracing for complex astrophysical high-opacity structuresOct 18, 2006The Morphology of M17-UC1 - A Disk Candidate Surrounding a Hypercompact HII RegionJan 8, 2007The Protostar in the massive Infrared Dark Cloud IRDC18223-3Apr 21, 2017TRUST I: A 3D externally illuminated slab benchmark for dust radiative transferJan 8, 2013The earliest phases of star formation - A Herschel key project. The thermal structure of low-mass molecular cloud cores