New observations from ESO's Very Large Telescope show for the first time a gas cloud being ripped apart
by the supermassive black hole at the center of the galaxy.
See images of new observations from ESO's Very Large Telescope showing a gas cloud ripped apart
by the supermassive black hole at the center of our galaxy, the Milky Way.
Maunakea, Hawaii — Stars forming in galaxies appear to be influenced
by the supermassive black hole at the center of the galaxy, but the mechanism of how that happens has not been clear to astronomers until now.
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.
Not exact matches
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.
Quasars are caused
by the close encounter of two
supermassive black holes, each with billions of solar masses and crammed into tight quarters
at the
center of a galaxy.
At the
center of our galaxy, in the immediate vicinity of its
supermassive black hole, is a region wracked
by powerful tidal forces and bathed in intense ultraviolet light and X-ray radiation.
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.
The
supermassive black hole at the
center of the Milky Way also betrays its presence
by its influence on nearby stars.
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.
Quasars are very luminous objects powered
by accretion of gas into
supermassive black holes at the
centers of distant galaxies.
On the evening of July 3, 2014, both of the mighty 10 - meter Keck Observatory telescopes were steered
by Dr. Andrea Ghez and her team of observers from the UCLA Galactic
Center Group to study the supermassive black hole at the center of our g
Center Group to study the
supermassive black hole at the
center of our g
center of our galaxy.
Most galaxies in the observable universe contain a
supermassive black hole at their
center, one that is either active and surrounded
by an accretion disk of dust, gas and other debris, or is dormant — lurking
at the
center, patiently awaiting its next meal.
This work is very meaningful since the possibility that a number of «stray
black holes» are floating around a
supermassive black hole at the Galactic
center was indicated
by the observational study for the first time.
By measuring the rapid orbits of the stars near the
center of our galaxy, Dr. Ghez and her colleagues have moved the case for a
supermassive black hole at the heart of the Milky Way from a possibility to a certainty.
An international research team led
by Takuma Izumi, a second - year master's student of science
at the University of Tokyo, and Kotaro Kohno, a professor
at the University of Tokyo, successfully captured a detailed image of high - density molecular gas around an active
supermassive black hole at the
center of a galaxy called NGC 1097
at the highest sensitivity ever achieved.
Figure 1 Composite image showing how powerful radio jets from the
supermassive black hole at the
center of a galaxy in the Phoenix Cluster inflated huge «bubbles» in the hot, ionized gas surrounding the galaxy (the cavities inside the blue region imaged
by NASA's Chandra X-ray observatory).
Quasars are among the most luminous objects in the universe, and generally are believed to be powered
by material being drawn into a
supermassive black hole at the
center of a galaxy, releasing large amounts of energy.
The predicted size of the shadow cast
by the event horizon of the
supermassive black hole at the
center of our own Milky Way is about 50 microarcseconds (that is one fifty millionth of an arcsecond, which is 1 / 3600th of a degree!).
This illustration provided
by Columbia University shows the
supermassive black hole Sagittarius A, located
at the
center of the Milky Way Galaxy, surrounded
by a cloud of dust and gas within which are 12 smaller
black hole...