Quark-Novae in massive binaries: a model for double-humped, hydrogen-poor, superluminous Supernovae
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/454/3/2353/4037664/stv2161.pdf
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1. Black Hole Formation via Hypercritical Accretion during Common‐Envelope Evolution
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1. The Macro-Physics of the Quark-Nova: Astrophysical Implications;Universe;2022-06-09
2. A Powerful e ± Outflow Driven by a Proto-strange Quark Star;The Astrophysical Journal;2021-12-01
3. A quark nova in the wake of a core-collapse supernova: a unifying model for long duration gamma-ray bursts and fast radio bursts;Research in Astronomy and Astrophysics;2020-03-01
4. Asymmetric core collapse of rapidly rotating massive star;Monthly Notices of the Royal Astronomical Society;2017-11-17
5. Simulating Hadronic-to-Quark-Matter with Burn-UD: Recent work and astrophysical applications;Journal of Physics: Conference Series;2017-06
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