The 3D structure of N132D in the LMC: a late-stage young supernova remnant
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Vogt, Frederic; Dopita, Michael
Description
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
Collections | ANU Research Publications |
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Date published: | 2011 |
Type: | Journal article |
URI: | http://hdl.handle.net/1885/64058 |
Source: | Astrophysics and Space Science |
DOI: | 10.1007/s10509-010-0479-7 |
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01_Vogt_The_3D_structure_of_N132D_in_2011.pdf | 2.52 MB | Adobe PDF | Request a copy |
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