Formation and Evolution of Dust in Type IIb Supernova with Application to the Cassiopeia A Supernova Remnant

Abstract

We investigate the formation of dust grains in the ejecta of a SN IIb and their evolution in the shocked gas in the SNR by considering the uniform and power-law density structures for the CSM. Based on these calculations, we also simulate the time evolution of thermal emission from the shock-heated dust in the SNR and compare the results with the observations of Cas A SNR. We find that the total mass of dust formed in the SN IIb is as large as 0.167 M_sun but the average radius of dust is smaller than 0.01 mum and is significantly different from those in SNe II-P with the massive H-envelope. In the explosion with the small-mass H-envelope, the expanding He core undergoes little deceleration, so that the gas density in the He core is too low for large-sized grains to form. In addition, the low-mass H-envelope of the SN IIb leads to the early arrival of the reverse shock at the dust-forming region. If the CSM is more or less spherical, therefore, the newly formed grains would be completely destroyed in the relatively dense shocked gas for the CSM density of n_H > 0.1 cm^{-3}. However, the actual CSM is likely to be non-spherical, so that a part of grains could be ejected into the ISM without being shocked. We demonstrate that the time evolution of the SED by thermal dust emission is sensitive to the ambient gas density and structure that affects the passage of the reverse shock into the ejecta. Thus, the SED evolution well reflects the evolution of dust through erosion by sputtering and stochastic heating. For Cas A, we consider the CSM produced by the steady mass loss of ~8x10^{-5} M_sun/yr during the supergiant phase. Then we find the infrared SED of Cas A is reasonably reproduced by thermal emission from the newly formed dust of 0.08 M_sun, which consists of 0.008 M_sun shocked warm dust and 0.072 M_sun unshocked cold dust.

50 pages, 17 figures, 3 tables. Accepted for publication in ApJ

References in corpus (21)

• The death of massive stars - I. Observational constraints on the progenitors of type II-P supernovae
• Dust Formation and Survival in Supernova Ejecta
• The Cassiopeia A Supernova was of Type IIB
• The Expansion Asymmetry and Age of the Cassiopeia A Supernova Remnant
• The Evolution of Dust in the Early Universe with Applications to the Galaxy SDSS J1148+5251
• Freshly Formed Dust in the Cassiopeia A Supernova Remnant as Revealed by the Spitzer Space Telescope
• Stellar sources of dust in the high redshift Universe
• Dust and the type II-plateau supernova 2004et
• Dust Destruction in the High-Velocity Shocks Driven by Supernovae in the Early Universe
• A Spitzer Space Telescope Study of SN 2003gd: Still No Direct Evidence that Core-Collapse Supernovae are Major Dust Factories
• Massive stars exploding in a He-rich circumstellar medium III. SN 2006jc: IR echoes from new and old dust in the progenitor CSM
• Aspherical Properties of Hydrodynamics and Nucleosynthesis in Jet-induced Supernovae
• Dust yields in clumpy SN shells: SN 1987A revisited
• Cassiopeia A: dust factory revealed via submillimetre polarimetry
• No cold dust within the supernova remnant Cassiopeia A
• Early Formation of Dust in the Ejecta of Type Ib SN 2006jc and Temperature and Mass of the Dust
• Spitzer IRAC Images and Sample Spectra of Cassiopeia A's Explosion
• Relative frequencies of supernovae types: dependence on host galaxy magnitude, galactocentric radius and local metallicity
• The Peculiar Type Ib Supernova 2006jc: A WCO Wolf-Rayet Star Explosion
• Properties of newly formed dust by SN2006jc based on near-to-mid infrared observation with AKARI
• Extinction curves flattened by reverse shocks in supernovae

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