They may have exotic structures such
as supermassive black holes at their centers.
Not exact matches
As matter falls toward the
supermassive black hole at the galaxy's
center, some of it is accelerated outward
at nearly the speed of light along jets pointed in opposite directions.
Over the past several decades, though, astronomers have realized that
black holes are not so unusual after all:
Supermassive ones, millions or billions of times
as hefty
as the sun, seem to reside
at the
center of most, if not all, galaxies.
The objects causing these low - frequency ripples — such
as orbiting
supermassive black holes at the
centers of distant galaxies — would be different from the higher frequency ripples, emitted by collisions of much smaller
black holes, that have so far been detected on Earth.
After charting stars in the heart of our galaxy traveling
at speeds up to 50 times faster than Earth circles the sun, scientists are convinced that a
supermassive black hole is pulling the strings,
as only the relentless grip of a
supermassive black hole could keep these frenzied stars locked into orbit within the galactic
center.
J1415 +1320 is what's known
as a blazar, a bright galaxy with a gluttonous
supermassive black hole at its
center (SN: 3/4/17, p. 13).
Resembling spotlights
at a Hollywood movie premier, such beams are probably generated
as matter plunges into a
supermassive black hole at the
center of the galaxy.
A small fraction of
supermassive black holes — the ginormous ones that lurk
at the
centers of galaxies — fire off light - speed jets of particles
as they snack.
Beginning in 1998, their groups have independently produced compelling evidence for the once controversial notion that our galaxy has
at its
center a
supermassive black hole which is about 4 million times
as massive
as the sun.
Researchers expect to directly measure this phenomenon beginning in the spring
as S0 - 2 makes its closest approach to the
supermassive black hole at the
center of our Milky Way galaxy.
«The electrons that make up the cloud initially bounce off the
supermassive black hole at the
center of one of the galaxies and accelerate
as a result.
The joint research team led by graduate student and JSPS fellow Takuma Izumi
at the Graduate School of Science
at the University of Tokyo revealed for the first time — with observational data collected by ALMA (Atacama Large Millimeter / submillimeter Array), in Chile, and other telescopes — that dense molecular gas disks occupying regions
as large
as a few light years
at the
centers of galaxies are supplying gas directly to the
supermassive black holes.
Supermassive black holes lurk at the centers of galaxies, and when those galaxies collide, eventually their supermassive black holes will first slowly circle each other spiraling inward like water down a drain, then eventually me
Supermassive black holes lurk
at the
centers of galaxies, and when those galaxies collide, eventually their
supermassive black holes will first slowly circle each other spiraling inward like water down a drain, then eventually me
supermassive black holes will first slowly circle each other spiraling inward like water down a drain, then eventually merge
as well.
The gas outflow driven by a
supermassive black hole at the galactic
center recently has become the focus of attention
as it possibly is playing a key role in the co-evolution of galaxies and
black holes.
VLBA images detect orbital motion of two
supermassive black holes as they circle each other
at the
center of a distant galaxy.
The discovery was made
as part of a program to detect
supermassive black holes, millions or billions of times more massive than the Sun, that are not
at the
centers of galaxies.
The position of the
supermassive black hole at the
center of our Milky Way galaxy,
as well
as the giant star S2, are shown (inset) in this near - infrared image from the European Southern Observatory's Very Large Telescope in Chile.
The halos around quasars — the brightest and the most active objects in the universe, they are galaxies formed less than 2 billion years after the Big Bang; they have
supermassive black holes in their
centers and consume stars, gas, interstellar dust and other material
at a very fast rate — are made of gas known
as the intergalactic medium and extend for up to 300,000 light - years from the
centers of the quasars.
From
supermassive black holes at galactic
centers to giant bursts of star formation to titanic collisions between galaxies, these discoveries allow astronomers to probe the current properties of galaxies
as well
as examine how they formed and developed.
The picture, pinned above his desk, shows a bright orange and yellow blob — the glow of cosmic gas
as it gets devoured by the
supermassive black hole at the
center of the galaxy.