activity
20032009
most citedFreshly Formed Dust in the Cassiopeia A Supernova Remnant as Revealed by the Spitzer Space Telescope

246 citations · 684 across the 11 of their papers we have counts for

collaborators

14 papers

astro-ph.GA2009

Dust Formation in the young core-collapse supernova remnant E0102

J. Rho, W. T. Reach, A. Tappe +4

We present Spitzer IRS and IRAC observations of the young supernova remnant E0102 (SNR 1E0102.2-7219) in the Small Magellanic Cloud. The infrared spectra show strong ejecta lines o…

astro-ph.GA200911 cited

Dust in Supernovae; Formation and Evolution

Takashi Kozasa, Takaya Nozawa, Nozomu Tominaga +3

Core--collapsed supernovae (CCSNe) have been considered to be one of sources of dust in the universe. What kind and how much mass of dust are formed in the ejecta and are injected…

astro-ph.SR20093 cited

Dust Formation Observed in Young Supernova Remnants with Spitzer

J. Rho, W. T. Reach, A. Tappe +8

We present dust features and masses observed in young supernova remnants (SNRs) with Spitzer IRS mapping and staring observations of four youngest supernova remnants: SNR 1E102.2-7…

astro-ph20081 cited

Origin and Nature of Dust in the Early Universe

T. Nozawa, T. Kozasa, H. Umeda +8

We present recent advances in theoretical studies of the formation and evolution of dust in primordial supernovae (SNe) that are considered to be the main sources of dust in the ea…

astro-ph2008

Evolution of newly formed dust in Population III supernova remnants and its impact on the elemental composition of Population II.5 stars

Takaya Nozawa, Takashi Kozasa, Asao Habe +5

We investigate the evolution of dust formed in Population III supernovae (SNe) by considering its transport and processing by sputtering within the SN remnants (SNRs). We find that…

astro-ph200883 cited

Early Formation of Dust in the Ejecta of Type Ib SN 2006jc and Temperature and Mass of the Dust

T. Nozawa, T. Kozasa, N. Tominaga +8

SN 2006jc is a peculiar supernova (SN), in which the formation of dust has been confirmed at an early epoch of ~50 days after the explosion. We investigate the possibility of such…