MEASURING DUST PRODUCTION IN THE SMALL MAGELLANIC CLOUD CORE-COLLAPSE SUPERNOVA REMNANT 1E 0102.2−7219

@article{Sandstrom2008MEASURINGDP,
  title={MEASURING DUST PRODUCTION IN THE SMALL MAGELLANIC CLOUD CORE-COLLAPSE SUPERNOVA REMNANT 1E 0102.2−7219},
  author={Karin M. Sandstrom and Alberto D. Bolatto and Sne{\vz}ana Stanimirovi{\'c} and Jacco Th. van Loon and J. D. T. Smith},
  journal={The Astrophysical Journal},
  year={2008},
  volume={696},
  pages={2138 - 2154}
}
We present mid-infrared spectral mapping observations of the core-collapse supernova remnant 1E 0102.2−7219 in the Small Magellanic Cloud using the InfraRed Spectrograph on the Spitzer Space Telescope. The remnant shows emission from fine structure transitions of neon and oxygen as well as continuum emission from dust. Comparison of the mid-IR dust emission with observations at X-ray, radio, and optical wavelengths shows that the dust is associated with the supernova ejecta and is thus newly… 

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References

SHOWING 1-10 OF 68 REFERENCES

Dust Destruction in Fast Shocks of Core-Collapse Supernova Remnants in the Large Magellanic Cloud

We report observations with the Multiband Imaging Photometer for Spitzer of four supernova remnants (SNRs) believed to be the result of core-collapse supernovae: N132D (0525-69.6), N49B (0525-66.0),

Freshly formed dust in the cassiopeia a supernova remnant as revealed by the Spitzer space telescope

We performed Spitzer Infrared Spectrograph mapping observations covering nearly the entire extent of the Cassiopeia A supernova remnant (SNR), producing mid-infrared (5.5-35 μm) spectra every 5″-10″.

Newly Synthesized Elements and Pristine Dust in the Cassiopeia A Supernova Remnant

Spectroscopic observations at 2.4-45 μm of the young supernova remnant Cas A with the Infrared Space Observatory (ISO) Short Wavelength Spectrometer reveal strong emission lines of O, Ne, Si, S, and

Multi-wavelength analysis of the dust emission in the Small Magellanic Cloud

We present an analysis of dust grain emission in the diffuse interstellar medium of the Small Magellanic Cloud (SMC). This study is motivated by the availability of 170� m ISOPHOT data covering a

Hubble Space Telescope Observations of Oxygen-rich Supernova Remnants in the Magellanic Clouds. II. Elemental Abundances in N132D and 1E 0102.2–7219*

We present Hubble Space Telescope (HST) Wide Field and Planetary Camera 2 images and Faint Object Spectrograph data of two young supernova remnants in the Magellanic Clouds, N132D (LMC) and 1E

Far-infrared observations of thermal dust emission from supernova 1987A

INFRARED observations of supernova 1987A are important for studying both the evolution of the ejecta and its interaction with the surrounding interstellar medium. Here we report observtions of

Molecules and dust production in the Magellanic Clouds

We present ESO/VLT spectra in the 2.9−4.1 μm range for a large sample of infrared stars in the Small Magellanic Cloud (SMC), mainly carbon stars, massive oxygen-rich Asymptotic Giant Branch (AGB)

Spitzer Space Telescope Detection of the Young Supernova Remnant 1E 0102.2?7219

We present infrared observations of the young, oxygen-rich supernova remnant 1E 0102.2-7219 (E0102) in the Small Magellanic Cloud, obtained with the Spitzer Space Telescope. The remnant is detected

No cold dust within the supernova remnant Cassiopeia A

Far-infrared and molecular line observations demonstrate that most of the detected submillimetre emission originates from interstellar dust in a molecular cloud complex located in the line of sight between the Earth and Cas A, and is therefore not associated with the remnant.

Dust in the Early Universe: Dust Formation in the Ejecta of Population III Supernovae

Dust grains play a crucial role in the formation and evolution history of stars and galaxies in the early universe. We investigate the formation of dust grains in the ejecta of Population III
...