Albireo is actually triple. The brighter yellow-colored
member, Albireo A, is a much closer double made of a third magnitude
(3.3) class K (K3) stable helium-fusing bright giant and a hotter
but dimmer (magnitude 5.5) class B (B9) hydrogen-fusing dwarf, the
two stars not readily separable in the telescope. The K giant has
a temperature of around 4400 Kelvin, a luminosity 950 times that
of the Sun, a radius 50 times solar, and a hefty mass of about 5
solar, while the close companion comes in at 11,000 Kelvin, 100
solar luminosities, and 3.2 solar masses. On average separated by
about 40 Astronomical Units, they take almost 100 years to go about
each other on a highly eccentric orbit.