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.
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3 Pith papers cite this work. 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.
SED modeling of early 2021 RS Oph data indicates bipolar ejecta with equatorial disk and confirms significant WD radiation originates from reprocessed shock emission explained by WD rotation.
citing papers explorer
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Pre-nova Observations of T CrB: A view from the CHARA Array
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.
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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.
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The first hours and days of the 2021 explosion of the recurrent symbiotic nova RS Ophiuchii
SED modeling of early 2021 RS Oph data indicates bipolar ejecta with equatorial disk and confirms significant WD radiation originates from reprocessed shock emission explained by WD rotation.