CHARA interferometry measures the red giant in T CrB at 0.70 mas (H-band) and 0.72 mas (K-band), giving a physical radius of 69-71 solar radii consistent with Roche lobe filling at the adopted distance.
Title resolution pending
4 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
representative citing papers
Detection of a micronova burst in TESS data of IGR J17014-4306, with inferred burned mass 1.6e-11 solar masses and recurrence time ~20 days, adding the eighth confirmed system.
A toy model of reverse shocks in novae predicts GeV gamma rays near optical peak and potential TeV emission later, consistent with Fermi observations under an empirically thin post-shock layer.
Long-term X-ray monitoring indicates Swift J174610.4-290018 is a recurrent nova similar to RS Oph rather than an accretion-disk corona source.
citing papers explorer
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Is the Peculiar Galactic Center Transient Swift J174610.4-290018 A Nova Outburst?
Long-term X-ray monitoring indicates Swift J174610.4-290018 is a recurrent nova similar to RS Oph rather than an accretion-disk corona source.