Not exact matches
Most scientists are sure that
in the centre of our galaxy there is a supermassive black hole; there are
binary systems where one of the
components is most likely a black hole.
Observations of the explosions of white dwarf stars
in binary systems, so - called Type Ia supernovae,
in the 1990s then led scientists to the conclusion that a third
component, dark energy, made up 68 % of the cosmos, and is responsible for driving an acceleration
in the expansion of the universe.
Finally, noncoplanarity between the
component stars of a
binary system should not have a significant impact on the stability of close -
in planetary orbits around each star (Alan Hale, 1994).
The primary
component in the
system is a spectroscopic
binary with the stellar classification of B2 IV, matching the spectrum of a blue - white subgiant star.