Active galactic nuclei (AGN) are a type of
extremely bright galaxy core seemingly fueled by powerful black holes actively gobbling large amounts of material.
Not exact matches
An unexpected opportunity to test this model came on June 3 when NASA's Swift Space Telescope picked up the
extremely bright gamma - ray burst, cataloged as GRB 130603B, in a
galaxy located almost 4 billion light - years away.
The
galaxies — which would appear as flat, rotating disks — are brimming with
extremely bright and massive blue stars.
And when quasars [
extremely bright, compact objects at the centers of some
galaxies] were discovered in the early 1960s, it was obvious that the source of power had to be gravitational because even nuclear power, which powers the stars, is too inefficient.
Extremely bright exploding stars, called superluminous supernovae, and long gamma ray bursts also occur in this type of
galaxy, he noted, and both are hypothesized to be associated with massive, highly magnetic and rapidly rotating neutron stars called magnetars.
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.
The first clue that supermassive black holes exist was the discovery several decades ago of quasars —
extremely bright objects in the centres of distant
galaxies.
Quasars are young
galaxies powered by massive black holes,
extremely bright,
extremely distant, and thus highly redshifted.
«It's
extremely bright, and it's probably larger than the Slug Nebula, but there's nothing else visible except the faint smudge of a
galaxy.
What the team directly observed was the last wave of Population III stars, suggesting that such stars should be easier to find than previously thought: they reside amongst regular stars, in
brighter galaxies, not just in the earliest, smallest, and dimmest
galaxies, which are so faint as to be
extremely difficult to study.
Few
galaxies have even more exotic nuclei, which are
extremely compact and
extremely bright, outshining their whole parent
galaxy; these are called quasars (an acronym for QUAsi-StellAR objects).
Therefore, the researchers consider that they managed to capture more like «normal»
galaxies, which had been impossible to detect up to now, than
extremely bright «submillimeter - luminous
galaxies».
Although GRB 000131, like other gamma - ray bursts, appears to have taken place in a remote «early
galaxy» (or «sub-galactic clumps» of stars) that is smaller than today's luminous
galaxies, astronomers found it difficult to detect that
extremely dim, sub-galactic clump of stars even with the Hubble Space Telescope, as the observed fading of the afterglow indicated that the maximum brightness of the gamma - ray emission was explosion was at least 10,000 times
brighter than its host
galaxy.
A new analysis of
galaxy colors, however, indicates that the farthest objects in the deep fields must be
extremely intense, unexpectedly
bright knots of blue - white, hot newborn stars embedded in primordial proto -
galaxies that are too faint to be seen even by Hubble's far vision — as if only the lights on a distant Christmas tree were seen and so one must infer the presence of the whole tree (more discussion at: STScI; and Lanzetta et al, 2002).
They were especially interested, and successful, in finding
extremely bright «novae» in other
galaxies, comparable to the one which had been observed in the Andromeda Galaxy M31 in 1885 (S Andromedae).