Sirius A & B
Sirius, designated Alpha Canis Majoris, is the brightest star in the night sky with a visual apparent magnitude of −1.46, almost twice as bright as Canopus, the next brightest star.
Its name is derived from a Greek word meaning "glowing".
Sirius appears so bright because of its intrinsic luminosity and its proximity to the Solar System, as at a distance of 8.6 ly it is one of Earth's nearest neighbors.
Sirius is in reality a binary star consisting of a bright white main-sequence star, twice as massive as the Sun (called Sirius A), and a faint white dwarf companion (termed Sirius B). The distance between the two varies between 8.2 and 31.5 astronomical units as they orbit every 50 years, which, seen from Earth, correspond to an apparent separation between 3 and 11 arcsec (text adapted from Wikipedia).At the time of the image their separation was closed to the maximum, which will be reached around 2025.
C14 +Siebert 1.5x (@ f/16) - Drizzle 1.5x - ZWO ASI290MM - iOptron CEM120 - Singapore