Not exact matches
Then in 1999, astrophysicists detected a steady buzz
of x-rays flowing from an object called Sagittarius A *, a
radio beacon at the
galaxy's
core — additional evidence for a black hole.
The black hole drives enormous outflows
of plasma from the
galaxy's
core which produce prodigious amounts
of radio emission.
They found that about 63 percent
of the background
radio emission comes from
galaxies with gorging black holes at their
cores and the remaining 37 percent comes from
galaxies that are rapidly forming stars.
Astronomers using the National Science Foundation's Very Long Baseline Array (VLBA)
of radio telescopes have discovered a cloud
of gas apparently being struck by a jet
of ultrafast particles powered by the energy
of a supermassive black hole at the
core of a
galaxy 450 million light - years away.
The
radio emission comes from the
core AND from very large regions on either side
of the optical part
of the
galaxy called «
radio lobes».
Astronomers using the National Science Foundation's Very Long Baseline Array
of radio telescopes have discovered a cloud
of gas apparently being struck by a jet
of ultrafast particles powered by the energy
of a supermassive black hole at the
core of a
galaxy 450 million light - years away.
New
radio images
of galaxies with bright quasar
cores show that, though the
galaxies appear normal in visible - light images, their gas has been disrupted by encounters with other
galaxies.
The «active» part
of the
galaxy is the supermassive black hole in its
core, which spews out strong jets
of energetic particles that produce enormous lobes
of radio emission.
Astronomer Vera Cooper Rubin found over decades
of radio observations that the rotational velocity
of clouds
of ionized hydrogen (HII regions) in spiral
galaxies like the Milky Way was not decreasing at increasing distance from their galactic
cores, like the velocity
of the planets around the Sun.