Most stars in our Milky Way galaxy are
members of binary systems.
Astronomers suspect that these stars may have originally been
members of binary systems.
«When we discovered this pulsar in 2009, we noticed that it was in the same direction as this massive star in the constellation Cygnus, but our initial measurements did not give any evidence that either star was
a member of a binary system,» Paul Ray, an astrophysicist at the Naval Research Laboratory in Washington, said, in a statement released Thursday.
Not exact matches
The
binary interaction model where a companion star is present is gaining traction because astronomers realize that at least 70 percent
of massive stars are
members of double - star
systems.
In the background is the star's
binary companion, Kepler - 13B, and the third
member of the multiple - star
system is the orange dwarf star Kepler - 13C.
In an eclipsing variable, one
member of a double, or
binary, star
system partially blocks the light
of its companion as it passes in front
of the latter, as observed from Earth.
When a star leaves the main sequence, its future evolution is precisely determined by its mass, rate
of rotation (or angular momentum), and chemical composition and whether it is a
member of a close
binary system.
Seen in the background is the star's
binary companion, Kepler - 13B, and the third
member of the multiple - star
system is the orange dwarf star, Kepler - 13C.
A typical X-ray
binary source consists
of a close double star
system in which one
member is a very compact object.
For example, if a black hole is a
member of a
binary star
system, matter flowing into it from its companion becomes intensely heated and then radiates X-rays copiously before entering the event horizon
of the black hole and disappearing forever.
At least 18 black widow and nine redback
binary systems have been found within the Milky Way so far, and additional
members of each class have been discovered within the dense globular star clusters that orbit our galaxy.