MAUNAKEA, Hawaii — Astronomers have uncovered evidence for a vast collection
of young galaxies 12 billion light years away.
Hydrogen emission from EGSY8p7 may indicate it is the first known example of an early generation
of young galaxies emitting unusually strong radiation.
The team compared the positions of these galaxies with the location of a cluster
of young galaxies 11.5 billion light - years from Earth in SSA22 which had been studied in visible light by the Subaru Telescope, operated by the National Astronomical Observatory of Japan (NAOJ).
Weighing in at 800 million solar masses, this supermassive specimen was found in the center
of a young galaxy that's generating powerful radiation.
Not exact matches
«Beware
of the dark side,» Yoda warned
young Luke Skywalker, and apparently the advice holds even in a
galaxy far, far away from the Star Wars universe.
The scientists found a desolate chunk
of space surrounding the center
of our
galaxy that is devoid
of young stars, which contradicts recent work done on the region.
The
young Welsh astronomer realized the alien had no chance
of seeing the Milky Way, let alone the universe's oodles
of dimmer
galaxies.
The field is so small that only a few foreground stars in the Milky Way lie within it; thus, almost all
of the 3,000 objects in the image are
galaxies, some
of which are among the
youngest and most distant known.
Many other potential applications
of this dataset are explored in the series
of papers, and they include studying the role
of faint
galaxies during cosmic reionisation (starting just 380,000 years after the Big Bang),
galaxy merger rates when the Universe was
young, galactic winds, star formation as well as mapping the motions
of stars in the early Universe.
Young star clusters and clouds
of hydrogen that formed in our
galaxy help trace the shapes
of the Milky Way's arms, so astronomers are reasonably certain that it has a spiral structure (see right).
Researchers also found that NGC 1448 has a large population
of young (just 5 million year old) stars, suggesting that the
galaxy produces new stars at the same time that its black hole feeds on gas and dust.
Instead, the bursts could come from a
young neutron star orbiting the dwarf
galaxy's dominant black hole, which probably has between 10,000 and 1 million times the mass
of the sun, he says.
«It appears that the
young stars in the early
galaxies like EGS - zs8 - 1 were the main drivers for this transition, called reionization,» said Rychard Bouwens
of the Leiden Observatory, co-author
of the study.
For example, astronomers have been trying to explain why some recently discovered distant, but
young,
galaxies contain massive amounts
of dust.
Using the Very Large Array
of the National Radio Astronomy Observatory in the US, the team observed radio emission from hydrogen in a distant
galaxy and found that it would have contained billions
of young, massive stars surrounded by clouds
of hydrogen gas.
The deep 3 - D map also revealed
young galaxies that existed as early as 12.5 billion years ago (at less than 10 percent
of the current universe age), only a handful
of which had previously been found.
«What our observations
of galaxies in the early universe tells us is these very early
young galaxies at the dawn
of the universe and their growing baby black holes already had some deep fundamental connection between them,» Schawinski said.
«Not only did we detect radio signals emitted by distant
galaxies when the Universe was three billion years
younger, but their gas reservoirs turned out to be unexpectedly large, about 10 times larger than the mass
of hydrogen in our Milky Way.
The remote object is part
of a discovery
of 22
young galaxies at ancient times located nearly at the observable horizon
of the universe.
But around the same time studies
of very distant
galaxies, which we see as they were when the Universe was very
young, were setting constraints on the amount
of baryonic matter in the Universe (New Scientist, Science, 30 April).
Note that regions
of Milky Way are blue from bursts
of star formation, while the
young, dead
galaxy is yellow, signifying an older star population and no new star birth.
And since the color and brightness
of young clusters gives their ages — and therefore, the time since a collision began — astronomers hope to put together a series
of snapshots
of the entire collision process by looking at many examples
of merging
galaxies.
Some stars in globular clusters may be 15 billion years old, he says, but the great bulge at the center
of the Milky Way — a
younger part
of the
galaxy, according to conventional wisdom — actually holds stars that are 1 or 2 billion years older.
The universe is turning out to be thronged with dim and ghostly
young galaxies that had escaped the notice
of astronomers.
Describing the discovery October 16 in Astrophysical Journal Letters, the team
of astronomers led by Arjen van der Wel
of the Max Planck Institute for Astronomy in Heidelberg, Germany report that the lensing
galaxy is relatively light,
young and bursting with new stars.
The evidence for
young massive
galaxies is the best yet, agrees astrophysicist Laura Ferrarese
of Rutgers University in Piscataway, New Jersey.
Aging red giant stars coexist with their more plentiful
younger cousins, the smaller, white, Sun - like stars, in this crowded region
of our
galaxy's ancient central hub, or bulge.
As Bregman hoped, dozens
of young stars turned up in each
of the three promising
galaxies — and as an added surprise, they even appeared in Messier 105.
The rate
of star formation is a small fraction
of what goes on in a
younger galaxy like the Milky Way, but even these low levels
of activity will force theorists to revise their models
of how
galaxies evolve.
The giant scope will also examine the composition
of matter in distant
young galaxies.
A team
of astronomers has doubled the number
of known
young, compact radio
galaxies —
galaxies powered by newly energized black holes.
To verify this rugby - scrimmage view
of the early universe, astronomers need to see even
younger, tinier proto -
galaxies, at about 90 percent
of the way back to the Big Bang.
Over the last few billion years, a mysterious kind
of «galactic warming» has caused many
galaxies to change from a lively place where new stars formed every now and then to a quiet place devoid
of fresh
young stars.
Astronomers have found a very
young galaxy that produces thousands
of stars a year — hundreds
of times more than our own Milky Way.
Young stars (yellow band) surrounding the core
of this dusty
galaxy show up in the NICMOS image (top), but not in the optical image.
He decided to point Hubble's Wide Field Camera 3, an addition made to the scope in 2009, at four nearby aging
galaxies to hunt for the telltale ultraviolet glow
of young stars.
While the new study adds to the Milky Way's tally
of star - forming regions, it may not substantially boost our
galaxy's star total because the
young, massive stars focused on in this study make up only a small percentage
of the overall population.
An international team studying gas clouds in a distant
galaxy has found that the temperature
of the gas matches almost exactly what models predicted for the
young cosmos.
The new findings suggest that many
young stars, our sun included, can migrate from one part
of the
galaxy to another.
Given this and other recent finds, astronomers either have been phenomenally lucky — or, more likely, they have underestimated substantially the number
of small, very
young galaxies in the early Universe.
A new study led by University
of California, Riverside astronomers casts light on how
young, hot stars ionize oxygen in the early universe and the effects on the evolution
of galaxies through time.
To make matters worse, the magnified object is a starbursting dwarf
galaxy: a comparatively light
galaxy (it has only about 100 million solar masses in the form
of stars [3]-RRB-, but extremely
young (about 10 - 40 million years old) and producing new stars at an enormous rate.
Other so - called hypervelocity stars are thought to have been boosted to their high speeds by close encounters with our
galaxy's supermassive black hole (see Hypervelocity stars: Catch them while you can), but this star is too
young to have travelled all the way from the centre
of the Milky Way.
The researchers mapped thousands
of star clusters in the attractive barred spiral
galaxy M83 (shown), 15 million light - years from Earth, finding that the percentage
of young stars in clusters declines from the urban core to the suburbs: Four thousand light - years from M83's center, 19 %
of young stars belong to clusters, whereas 13,000 light - years out, just 7 % do.
Neal Evans, an astronomy professor at the University
of Texas at Austin, credits the researchers for broadening the observational window from the somewhat anomalous luminous events to include run -
of - the - mill
galaxies in the fairly
young universe.
Like any spiral
galaxy, M106 has a pair
of arms full
of bright
young stars (green), but researchers have long wondered at the source
of its two extra arms (purple and blue), visible in radio and X-ray images.
Astronomers have seen them shooting out
of young stars just being formed, X-ray binary stars and even the supermassive black holes at the centers
of large
galaxies.
[4] Very little is known about the origin and characteristics
of the magnetic fields that were present in our
galaxy when it was
young, so it is unclear whether they have grown stronger over time, or decayed.
In lieu
of a working time machine, we learn about the birth
of our Sun and its planets by studying
young stars in our
galaxy.
The newfound
young star clusters lie thousands
of light - years below the plane
of our Milky Way
galaxy, a flat spiral disk seen in this artist's conception.