Quark-novae in neutron star - white dwarf binaries: a model for luminous (spin-down powered) sub-Chandrasekhar-mass Type Ia supernovae?
Author:
Publisher
IOP Publishing
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/1674-4527/13/i=4/a=006/pdf
Reference194 articles.
1. Equation of state of nucleon matter and neutron star structure
2. Color-flavor locking and chiral symmetry breaking in high density QCD
3. Quark matter in compact stars?
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1. The Macro-Physics of the Quark-Nova: Astrophysical Implications;Universe;2022-06-09
2. 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
3. Quark-Novae in massive binaries: a model for double-humped, hydrogen-poor, superluminous Supernovae;Monthly Notices of the Royal Astronomical Society;2015-10-13
4. THE SUPERLUMINOUS SN DES13S2cmm AS A SIGNATURE OF A QUARK-NOVA IN A HE-HMXB SYSTEM;The Astrophysical Journal;2015-08-19
5. THE PUZZLING EARLY DETECTION OF LOW VELOCITY56Ni DECAY LINES IN SN 2014J: HINTS OF A COMPACT REMNANT;The Astrophysical Journal;2015-03-04
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