Its central star is a symbiotic Mira variable - white dwarf pair.

It is a Mira variable with an apparent visual magnitude of approximately 10.9.

It is also a Mira variable with a period of 407.6 days, and has one of the largest magnitude ranges known (from 4.7 to 14.3).

It is a Mira variable that pulsates with a 420-day cycle, and varies in radius from 1.9 to 2.3 astronomical units.

A few Mira variables are also known to be natural maser sources.

He also pursued his research on Mira variables, also known as Long period variable stars.

At least three red giants are Mira variables in Canis Minor.

Here we have another S-type Mira variable, with a period of 407 days.

It is a Mira variable with an apparent visual magnitude which varies between 9.3 and 15.8.

It is classified as a Mira variable and its brightness varies from magnitude +5.3 to +11.8 with a period of 546.2 days.