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
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
years
2026 2representative citing papers
Statistical analysis of T CrB light curves finds no robust orbital-phase locking for active phases or eruptions.
citing papers explorer
-
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.
-
Lack of Significant Orbital-Phase Locking in the Active Phases of the Recurrent Nova T CrB
Statistical analysis of T CrB light curves finds no robust orbital-phase locking for active phases or eruptions.