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.
This star emits 2,460 times the luminosity of the Sun from its photosphere at an effective temperature of 16,550 K. It shares characteristics with both short-period B-type variables and Cepheid variables.