HD 40873

HD 40873 is a star in the northern constellation of Auriga, a few degrees to the south of Delta Aurigae. Located around 455 light-years distant, it shines with a luminosity approximately 38 times that of the Sun and has an effective temperature of 7,753 K. It is a suspected variable star and has a fairly rapid rotation rate, showing a projected rotational velocity of 134 km/s. Eggen (1985) suggested it is a probable member of the Hyades Supercluster.

HD 40873

HD 40873 is a star in the northern constellation of Auriga, a few degrees to the south of Delta Aurigae. Located around 455 light-years distant, it shines with a luminosity approximately 38 times that of the Sun and has an effective temperature of 7,753 K. It is a suspected variable star and has a fairly rapid rotation rate, showing a projected rotational velocity of 134 km/s. Eggen (1985) suggested it is a probable member of the Hyades Supercluster.