[AAVSO LightCurve, 1yr]
[AAVSO LightCurve, 5yr]
GCVS data:
Epoch 2000: ra = 111.345, dec = -3.597
Variability type: *
Spectral type: M4ep+F0II-III
GCVS remarks:
Usually was considered as mira type variable [09421]. In the Table the epoch of light maximum and the period are given according to [09419]. According to [09420] the Balmer emission lines originate in the nebulosity surrounding the symbiotic system and are excited by the hot component, and light variations are due to the orbital motion in the system.
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Chart status: UNCHECKED