A source known as iPTF14hls, assumed to be a Type IIP supernova, may be a long-term outflow similar to stellar winds, according to a new study published November 5 on arXiv.org. The new research proposes that iPTF14hls is most likely a so-called "hyper-wind"--an extreme mass outflow from a massive star.
IPTF14hls may be a variable hyper-wind from a very massive star, study suggests
Phys.org - 14 Nov 2019 16:00
A source known as iPTF14hls, assumed to be a Type IIP supernova, may be a long-term outflow similar to stellar winds, according to a new study published November 5 on arXiv.org. The new research proposes that iPTF14hls is most likely a so-called "hyper-wind"--an extreme mass outflow from a massive star.
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