Showing 1–20 of 25 results
/ Date/ Name
Jul 6, 2003Dust in the Early Universe: Dust Formation in the Ejecta of Population III SupernovaeMar 2, 2009Dust in Supernovae; Formation and EvolutionJan 15, 2010Effects of grain shattering by turbulence on extinction curves in starburst galaxiesOct 16, 2008Spitzer Spectral Mapping of Supernova Remnant Cassiopeia AJun 4, 2007Evolution of Dust in Primordial Supernova Remnants: Can Dust Grains Formed in the Ejecta Survive and be Injected into the Early Interstellar Medium?Jun 25, 2005A model for the infrared dust emission from forming galaxiesApr 5, 2011The Role of Dust in the Early Universe I : Protogalaxy EvolutionMay 23, 2011On the effects of microphysical grain properties on the yields of carbonaceous dust from type II SNeJun 4, 2010The Three-Dimensional Structure of Interior Ejecta in Cassiopeia A at High Spectral ResolutionOct 6, 2009AKARI Infrared Observations of the Supernova Remnant G292.0+1.8: Unveiling Circumstellar Medium and Supernova EjectaNov 17, 2010The Three-Dimensional Structure of Cassiopeia AAug 20, 2012Nucleosynthetic Layers in the Shocked Ejecta of Cassiopeia ASep 7, 2015Probing the Physical Conditions of Supernova Ejecta with the Measured Sizes of Presolar Al2O3 GrainsSep 23, 2009Formation and Evolution of Dust in Type IIb Supernova with Application to the Cassiopeia A Supernova RemnantSep 25, 2008Evolution of newly formed dust in Population III supernova remnants and its impact on the elemental composition of Population II.5 starsSep 29, 2011Formation of SiC Grains in Pulsation-Enhanced Dust-Driven Wind Around Carbon Rich Asymptotic Giant Branch StarsAug 1, 2012Can the Growth of Dust Grains in Low-Metallicity Star-Forming Clouds Affect the Formation of Metal-Poor Low-Mass Stars?Apr 22, 2014Dust Production Factories in the Early Universe: Formation of Carbon Grains in Red-supergiant Winds of Very Massive Population III StarsAug 8, 2013Formulation of Non-steady-state Dust Formation Process in Astrophysical EnvironmentsDec 6, 2016Dust formation and mass loss around intermediate-mass AGB stars with initial metallicity $Z_{\rm ini} \leq 10^{-4}$ in the early Universe I: Effect of surface opacity on the stellar evolution and dust-driven wind