Showing 1–17 of 17 results
/ Date/ Name
Jan 1, 2019The CARMA-NRO Orion Survey: The filamentary structure as seen in C$^{18}$O emissionMar 14, 2006High-resolution mapping of interstellar clouds with near-infrared scattered lightJul 18, 2002Dust emission from inhomogeneous interstellar clouds: radiative transfer in 3D with transiently heated particlesAug 5, 2020From the CMF to the IMF: Beyond the Core-Collapse ModelFeb 18, 2003Photoelectric heating and [CII] cooling in translucent clouds: results for cloud models based on simulations of compressible MHD turbulenceAug 12, 2007A Corona Australis cloud filament seen in NIR scattered light I. Comparison with extinction of background starsSep 23, 2010Accuracy of core mass estimates in simulated observations of dust emissionSep 5, 1997Dark galaxies, spin bias and gravitational lensesApr 17, 2001Cooling Rates of Molecular Clouds Based on Numerical MHD Turbulence and non-LTE Radiative TransferAug 18, 2004Multi-Resolution Radiative Transfer for Line EmissionSep 6, 2006Simulations of polarized dust emissionSep 9, 2013Zooming in on the Formation of Protoplanetary DisksJan 7, 2009Predictions of polarized dust emission from interstellar clouds: spatial variations in the efficiency of radiative torque alignmentDec 19, 2018Expanding associations in the Vela-Puppis region: 3D structure and kinematics of the young populationNov 14, 2023Evaporation Ages: a New Dating Method for Young Star ClustersJan 20, 1997The ages and distances of globular clusters with the luminosity function method: the case of M5 and M55Dec 8, 1999Radiative Transfer in 3D