The quantity and composition of dust produced in core-collapse supernovae is a matter of much debate. Observations of dust around quasars at high redshift have been explained via models invoking efficient dust production, with typical yields of 0.1-1 msol\ of dust per supernova. Observations of supernovae and their remnants, however, have yet to provide evidence for efficient dust production. Observations by Stanimirovic et al. (2005) of the young, oxygen rich, supernova remnant 1E 0102.2-7219 in the Small Magellanic Cloud placed an upper limit on the dust produced in the supernova of 8Ã 10-4 msol, far less than the amount predicted by models. We present 5-35 micron IRS spectral mapping observations of SNR E 0102 obtained as part of the Sp...
International audienceWe present the analysis of supernova remnants (SNRs) in the Large Magellanic C...
We have used the instruments on the Spitzer Space Telescope to study the Large Magellanic Cloud supe...
With the entire Small Magellanic Cloud (SMC) mapped by the Spitzer Space Telescope and Herschel Spac...
We present dust features and masses observed in young supernova remnants (SNRs) with Spitzer Infrare...
The importance of supernovae as a source of interstellar dust has long been debated. Theoretical mod...
This thesis presents the first population study of supernova remnants (SNRs) in one whole galaxy – t...
Aims: We present a comprehensive study of the supernova remnant (SNR) population of the Small Magell...
We investigate the dust associated with the supernova remnant (SNR) N49 in the Large Magellanic Clou...
We present dust features and masses observed in young supernova remnants (SNRs) with Spitzer Infrar...
International audienceWe present the analysis of supernova remnants (SNRs) in the Large Magellanic C...
We have used the instruments on the Spitzer Space Telescope to study the Large Magellanic Cloud supe...
With the entire Small Magellanic Cloud (SMC) mapped by the Spitzer Space Telescope and Herschel Spac...
We present dust features and masses observed in young supernova remnants (SNRs) with Spitzer Infrare...
The importance of supernovae as a source of interstellar dust has long been debated. Theoretical mod...
This thesis presents the first population study of supernova remnants (SNRs) in one whole galaxy – t...
Aims: We present a comprehensive study of the supernova remnant (SNR) population of the Small Magell...
We investigate the dust associated with the supernova remnant (SNR) N49 in the Large Magellanic Clou...
We present dust features and masses observed in young supernova remnants (SNRs) with Spitzer Infrar...
International audienceWe present the analysis of supernova remnants (SNRs) in the Large Magellanic C...
We have used the instruments on the Spitzer Space Telescope to study the Large Magellanic Cloud supe...
With the entire Small Magellanic Cloud (SMC) mapped by the Spitzer Space Telescope and Herschel Spac...