Doppler tomography of the symbiotic recurrent nova T CrB during its super-active phase resolves a bright spot, disk wind, irradiated giant surface, and an accelerating nebula, supporting a dwarf-nova-like disk-instability origin.
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Resolving the mass transfer in the symbiotic recurrent nova T Coronae Borealis
Doppler tomography of the symbiotic recurrent nova T CrB during its super-active phase resolves a bright spot, disk wind, irradiated giant surface, and an accelerating nebula, supporting a dwarf-nova-like disk-instability origin.