The 3D structure of N132D in the LMC: a late-stage young supernova remnant
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Vogt, Frederic
Dopita, Michael
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Kluwer Academic Publishers
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We have used the Wide Field Spectrograph (WiFeS). on the 2.3 m telescope at Siding Spring Observatory to map the [O III] 5007 Å dynamics of the young oxygen-rich supernova remnant N132D in the Large Magellanic Cloud. From the resultant data cube, we have
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Astrophysics and Space Science
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2037-12-31
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