Quasars are
bright disks of gas and dust swirling around supermassive black holes.
In 1611, less than two years after Galileo began examining the skies, German astronomer Christoph Scheiner spotted something silhouetted against
the bright disk of the sun.
Like other spiral galaxies, the Milky Way Galaxy, has
a bright disk of stars with sweeping arms of conspicously younger, brighter, and bluer stars enveloped in gas and dust that curve around its center like the arms of a huge pinwheel.
A coronagraph is designed to look at the solar atmosphere by blocking out
the bright disk of the sun.
Not exact matches
Six months from now, we will have 24 hours
of daylight and the moon will be a pale
disk in the blue sky, growing
brighter each month as we move back toward winter again.
No space probe or telescope built by humans has ever escaped the Milky Way to turn back and take a portrait; because we are embedded in our galaxy's
disk, we can only see it as a
bright band
of stars across the sky.
Theorists speculate that so - called quasi-periodic oscillation was caused by
bright blobs in the black hole's accretion
disk, made up
of gas that slowly spirals towards the hole.
Scientists observe coronal mass ejections using a type
of instrument called a coronagraph, in which a solid
disk blocks the sun's
bright face, revealing the sun's tenuous atmosphere, called the corona.
The western side (tilted closer to the Earth) appears
brighter in polarized light, while in total intensity the eastern side appears slightly
brighter, particularly just to the east
of the widest apparent separation points
of the
disk.
This visible - light image taken by NASA's Hubble Space Telescope reveals a pancake - shaped
disk of gas around an extremely
bright star in our Milky Way galaxy.
Reconciling this complex and apparently - contradictory pattern
of brighter and darker regions required a major overhaul
of our understanding
of this circumstellar
disk.
Massive numbers
of comets may even produce the
bright debris
disks seen around other stars.
In addition to accretion
disks, black holes also have winds and incredibly
bright jets erupting from them along their rotation axis, shooting out matter and radiation at nearly the speed
of light.
Cygnus X-1 was found as part
of a binary star system in which an extremely hot and
bright star called a blue supergiant formed an accretion
disk around an invisible object.
It's also possible, he says, that the magnetic field is sucking power out
of the accretion
disk, making it appear less
bright.
Bañados was looking in particular for quasars — some
of the
brightest objects in the universe, that consist
of a supermassive black hole surrounded by swirling, accreting
disks of matter.
The accretion
disks around supermassive black holes (black holes with masses millions
of times that
of the Sun) are some
of the
brightest objects in the Universe.
But rather than a uniform field
of random ejections, they saw
bright jets
of atoms shooting together from the rim
of the
disk, like miniature fireworks.
The team found that
bright stars are mainly located in the inner
disk of M81, while most
of the young stars in outlying concentrations are fainter and have similar luminosity distributions as that
of the stellar stream between M81 and NGC 3077.
Spirals have most
of their
bright stars, gas, and obscuring dust in a thin
disk.
«Astronomers know star formation has just completed in this region, called Upper Scorpius, because roughly a quarter
of the stars still have
bright protoplanetary
disks,» David said.
In 2010 we began a near - infrared (NIR) spectral survey
of bright debris
disks with reported IRAS excesses and optically resolved
disks.
The
bright spiral
disk may also be surrounded by a much fainter, outer ring
of stars, possibly stripped from at least one, former satellite galaxy.
The problem,
of course, stems from the fact that with the exception
of active black holes — which are surrounded with a
bright accretion
disk — it is kind
of hard to hunt down objects that do not allow even light to escape their gravitational pull.
But that doesn't mean astronomers can't see them;
bright X-ray light streams from the superhot
disk of material spiraling into a black hole's mouth.
With this, two new phenomena have been discovered: the fast flares in the early light curve seen from days 9 - 15 (which have no proposed explanation) and the optical dips seen out
of eclipse from days 41 - 61 (likely caused by raised rims
of the accretion
disk occulting the
bright inner regions
of the
disk as seen over specific orbital phases).
Abstract: We present $ H$ - band scattered light imaging
of a
bright debris
disk around the A0 star HD 36546 obtained from the Subaru Coronagraphic Extreme Adaptive Optics (SCExAO) system with data recorded by the HiCIAO camera using the vector vortex coronagraph.
M82 is remarkable for its
bright blue
disk, webs
of shredded clouds, and fiery - looking plumes
of glowing hydrogen blasting out
of its central regions.
The dark
disks are seen in these images because they are silhouetted against the
bright backdrop
of the hot gas
of the Orion nebula.
At these wavelengths, astronomers can peer at the
disks of gas and dust around newborn stars, see into star - forming clouds, and observe early galaxies that are
bright in submillimetre wavelengths but obscured by dust in optical light.
Indeed, GRBs appear to emit produce even more energy than supernovae or even quasars (which are energetically
bright accretion
disks and bi-polar jets around supermassive black holes that are most commonly found in the active nuclei
of some distant galaxies and possibly even in the pre-galaxy period after the Big Bang).
Seen in infrared light, the faint starlight gives way to the glowing
bright patterns
of dust found throughout the galaxy's
disk (Credit: NASA / JPL - Caltech / J.
«This lack
of collisionality distinguishes the Sagittarius A * accretion
disk from
brighter and more radiative
disks that orbit other black holes,» the Princeton Plasma Physics Laboratory (PPPL) explained in the statement.
As a result, some accretion
disks around supermassive black holes are incredibly
bright, and can outshine all the billions
of stars in their host galaxy put together.
The separate
disks lay so perfectly that the necklace seems to drape along the lines
of your collarbones, and the
bright yellow hue is just the right amount
of sass.
The first sign
of trouble appears in the Windows Store's Spotlight section: Are apps like «Periodic Table» and «
Disk Falcon» really the best and
brightest Microsoft has to offer one month before launch?
We find that most
of the solar cycle variation in the total solar irradiance can be accounted for by the absolute magnetic field strength on the solar
disk, if fields associated with dark and
bright regions are considered separately.