Showing 1–20 of 69 results
/ Date/ Name
Sep 28, 20042-D Models of Protostars: III. Effects of Stellar TemperatureJun 23, 20052-D and 3-D Radiation Transfer Models of High-Mass Star FormationApr 26, 2011Monte Carlo Radiative TransferMar 21, 20032-D Radiative Transfer in Protostellar Envelopes: I. Effects of Geometry on Class I SourcesAug 30, 20032-D Radiative Transfer in Protostellar Envelopes: II. An Evolutionary SequenceAug 11, 2006Interpreting Spectral Energy Distributions from Young Stellar Objects. I. A grid of 200,000 YSO model SEDsMay 1, 2010Spitzer Analysis of HII Region Complexes in the Magellanic Clouds: Determining a Suitable Monochromatic Obscured Star Formation IndicatorMar 9, 2009The Mass-Loss Return From Evolved Stars to the LMC: Empirical Relations for Excess Emission at 8 and 24 μmMay 23, 2022The SOFIA Massive (SOMA) Star Formation Survey. IV. Isolated ProtostarsJan 5, 2011Fundamental parameters, integrated RGB mass loss and dust production in the Galactic globular cluster 47 TucanaeMar 11, 2004The Structure of Brown Dwarf Circumstellar DisksMay 28, 2013Effects of diffuse background emission and source crowding on photometric completeness in Spitzer Space Telescope IRAC surveys: The GLIMPSE Catalogs and ArchivesFeb 15, 2013A Massive Protostar Forming by Ordered Collapse of a Dense, Massive CoreOct 2, 2009Warm and Dense Molecular Gas in the N159 Region: 12CO J=4-3 and 13CO J=3-2 Observations with NANTEN2 and ASTESep 17, 2012The Structure of Pre-transitional Protoplanetary Disks I: Radiative Transfer Modeling of the Disk+Cavity in the PDS 70 systemJun 11, 2020The SOFIA Massive (SOMA) Star Formation Survey. III. From Intermediate- to High-Mass ProtostarsDec 15, 2010A Panchromatic View OF NGC 602: Time-Resolved Star Formation with the Hubble and Spitzer Space TelescopesJul 15, 2008Emission from Very Small Grains and PAH Molecules in Monte Carlo Radiation Transfer Codes: Application to the Edge-On Disk of Gomez's HamburgerNov 27, 2007Panchromatic Spectral Energy Distributions of Dusty Galaxies with RADISHE. I. Predictions for Herschel: Correlating Colors with Galactic Energy SourcesJun 24, 2011Surveying the Agents of Galaxy Evolution in the Tidally-Stripped, Low Metallicity Small Magellanic Cloud (SAGE-SMC) II. Cool Evolved Stars