Very deep inside the SN 1987A core ejecta: Molecular structures seen in 3D
Most massive stars end their lives in core-collapse supernova explosions and enrich the interstellar medium with explosively nucleosynthesized elements. Following core collapse, the explosion is subject to instabilities as the shock propagates outward through the progenitor star. Observations of the...
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| Fformat: | Journal article |
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American Astronomical Society
2017
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