«We're seeing a new class of
stars near the black hole, and as a consequence of the black hole.»
Not exact matches
The group observed the colossal winds of material — or outflows — that originate
near the supermassive
black hole at the heart of the pair's southern galaxy, and have found the first clear evidence that
stars are being born within them [1].
Images of M32, a dwarf elliptical galaxy
near to our own, show that
stars become clustered much more closely together
near its centre, which is what should happen if the galaxy contains a
black hole.
One theory suggests the
stars were pulled from a pre-existing
star cluster that happened to wander
near the
black hole.
A sun - size
star approaching within 30 solar radii of the monster, they calculate, would be ripped apart by the
black hole's gravitational pull, which would be far stronger on the
near side of the
star than on the far side.
A
star ripped to shreds by a massive
black hole may explain a strange feature
near the center of our galaxy.
Hints of their existence came from either X-ray emissions — thought to arise as the
black holes consumed their companion
stars — or the motion of
stars near the centre of some clusters (see Middleweight
black holes are «missing link»).
SIM will also measure the motions of
stars near the center of many galaxies, which should tell us whether they harbor enormous
black holes at their core.
Based on data taken by NASA's Chandra X-ray Observatory, the model takes into account how energy flows between two regions around the
black hole — an inner core close to the boundary beyond which light can not escape (the event horizon) and an outer ring that extends far out and includes the massive young
stars lurking
near the
black hole.
The finding suggests that mature
stars found
near the
black hole by other researchers may have originated there despite the violent conditions, says Ramírez, who presented her findings at a press conference on Wednesday.
Scary, but not terribly likely: We are not close to a
star about to go supernova, and we're a long way from the
nearest black hole.
The new images home in on a region around the
black hole less than 4.2 light - years across — smaller than the distance between the sun and its
nearest star, says Roopesh
To limit inherent systematic uncertainties, Ghez's group accounted for overlapping light sources when one
star passes in front of another or
near the
black hole itself, where infalling material emits radiation.
«Infant
stars found surprisingly
near galaxy's supermassive
black hole: Earliest phase of
star formation ever observed in highly hostile environment.»
Observations with the Very Large Array
near Socorro, New Mexico, revealed two objects whose radio spectra resemble those of other
black hole systems located outside of
star clusters.
In the new study, Charles Hailey, an astrophysicist at Columbia University, and his colleagues scrutinized the past dozen years of data gathered by the Chandra X-ray Observatory, an orbiting craft whose instruments are designed to detect high - energy radiation emitted by the immensely hot material surrounding exploded
stars and
near black holes.
Instead, the X-ray data show the gas
near the
black hole likely originates from winds produced by a disk - shaped distribution of young massive
stars.
ALMA discovers remarkably early signs of low - mass
star formation
near the supermassive
black hole at the center the Milky Way.
The blue
stars surrounding the
black hole are no more than 200 million years old, and therefore must have formed
near the
black hole in an abrupt burst of
star formation.
The velocities of the
stars near its nucleus suggested the presence of a
black hole as early as 1984.
The orbits of two
stars, S0 - 2 and S0 - 38 located
near the Milky Way's supermassive
black hole will be used to test Einstein's theory of General Relativity and potentially generate new gravitational models.
Ghez used this cutting - edge system to track the orbits of
stars near the supermassive
black hole located at the center of the Milky Way.
Before the heavens were stretched out, those
stars had high velocities, because they were
near a galaxy's center of mass where a
black hole was growing.
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.
Based on their observations, they have concluded that the rate of a TDE occurring increases «dramatically» when two galaxies are colliding, most likely due to the fact that such events cause a large number of
stars to be formed
near the central supermassive
black holes of the merging systems.
When a
black hole is created from a supernova from a massive
star or a collision between neutron
stars (or a neutron
star with a
black hole), one of a pair of bi-polar jets of gamma rays travelling at
near light - speed may be directed at the Earth (more).
A group of astronomers in Germany and the Czech Republic observed three
stars in a cluster
near the supermassive
black hole at the center of the Milky Way galaxy.
u «Ironically,
stars such as these have no business being so close to a
black hole... there is no plausible explanation of how and why the hot, young
stars near the centre of the Milky Way and Andromeda got there.»
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 astronomers also noticed that one side of the donor
star was always brighter than the other because it was illuminated by X-rays coming from
near the
black hole.
Archival Hubble images, taken by the
Near Infrared Camera and Multi-Object Spectrometer (NICMOS), support the idea of twin
black holes pushing
stars away.