Enhanced mass transfer events trigger the nova eruptions in T CrB by building 95% of the ignition envelope mass on a 1.29 solar-mass white dwarf via a high-viscosity disk.
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2 Pith papers cite this work, alongside 3 external citations. Polarity classification is still indexing.
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New NuSTAR observation and historical review indicate an initial strong shock near the red giant in RS Oph produces both gamma-ray particle acceleration and 0.2-30 keV thermal X-rays, with gamma-ray flux from Fermi inconsistent and implications for T CrB.
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The accretion-driven eruption of the recurrent nova T Corona Borealis
Enhanced mass transfer events trigger the nova eruptions in T CrB by building 95% of the ignition envelope mass on a 1.29 solar-mass white dwarf via a high-viscosity disk.
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The powerful shocks in RS Oph: NuSTAR X-ray data and a complete review
New NuSTAR observation and historical review indicate an initial strong shock near the red giant in RS Oph produces both gamma-ray particle acceleration and 0.2-30 keV thermal X-rays, with gamma-ray flux from Fermi inconsistent and implications for T CrB.