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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Bibliografische gegevens
Hoofdauteurs: Abellan, FJ, Indebetouw, R, Marcaide, JM, Roche, P, Et al.
Formaat: Journal article
Gepubliceerd in: American Astronomical Society 2017