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.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
astro-ph.HE 2years
2026 2representative citing papers
Statistical tests on outburst timings from AAVSO and historical data show no significant orbital-phase preference for active phases in T CrB.
citing papers explorer
-
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.
-
Lack of Significant Orbital-Phase Locking in the Active Phases of the Recurrent Nova T CrB
Statistical tests on outburst timings from AAVSO and historical data show no significant orbital-phase preference for active phases in T CrB.