It is radiating 2,460 times the luminosity of the Sun from its photosphere at an effective temperature of 16,550 K. This star is notable as demonstrating similarities between the short-period B-type variables and the Cepheid variables.
It is emitting 2,460 times the Sun's luminosity from its photosphere at an effective temperature of 16,550 K. This star stands out as exhibiting similarities between short-period B-type variables and Cepheid variables.