An artist's impression shows a primordial quasar as it might have been, surrounded by sheets of gas, dust, stars and
early star clusters.
Not exact matches
When the cosmos was a few hundred million years old, this gas coalesced into the
earliest stars, which formed in
clusters that clumped together into galaxies, the oldest of which appears 400 million years after the universe was born.
Astronomers had long debated whether globular
clusters were massive enough for black holes to form, either when the
clusters condensed in the
early universe or when gas and
stars accumulated at their cores.
Current theories suggest that the seeds of these black holes were the result of either the growth and collapse of the first generation of
stars in the Universe; collisions between
stars in dense stellar
clusters; or the direct collapse of extremely massive
stars in the
early Universe.
The research, also posted online at arXiv.org, negates an
earlier finding that
stars were separated from their dark matter in Abell 3827, a
cluster including four colliding galaxies about 1.3 billion light - years from Earth (SN: 5/16/15, p. 10).
Stars in the extremely old globular cluster NGC 6397 are slightly polluted by the shattered fusion products of an even earlier generation of s
Stars in the extremely old globular
cluster NGC 6397 are slightly polluted by the shattered fusion products of an even
earlier generation of
starsstars.
Earlier observations of
star clusters forming in evenly distributed clumps in spiral galaxies could explain Tremblay's «serendipitous discovery» in the Hubble data.
Early on, when the
cluster begins to condense from a collapsing cloud of gas, the brightest and shortest - lived
stars blow out fierce winds that energize the first set of cosmic rays and expel material from the
star itself.
Both spots are dense
clusters with conditions like those of the
early universe, so this could help reveal how some of the very first
stars formed.
As shown in the zoom - in panel at right, dense
clusters in the low - metallicity Magellanic Clouds, which better resemble conditions in the
early history of the Milky Way, can not be resolved into individual
stars for
star - count IMFs or UV - derived mass - accretion rates.
Up to half of
early breast cancers contain little
clusters of microcalcifications, tiny deposits of calcium that on a mammogram look like a constellation of faint
stars.
This sample is now providing the best measurement yet of when and how fast galaxy
clusters stop forming
stars in the
early Universe.
Early in 1765, he found the
star cluster M41.
This portion of the spectrum, which is more energetic than most radio waves yet less energetic than visible and infrared light, holds the key to understanding a great variety of fundamental processes, including planet and
star formation, and the formation and evolution of galaxies and galaxy
clusters in the
early Universe.
The additional 42 entries were mostly discovered
earlier, and most of them (32) are open
star clusters; there are no planetary nebulae, supernova remnants, elliptical and lenticular galaxies among them, and the only spiral galaxy in this list is our own, the Milky Way.
Such a view would yield a treasure trove of information from which to deduce the
early history of structure formation, and the origin of the
stars, galaxies,
clusters and quasars that we see today.
It will be used for many different types of astronomical studies ranging from detailed imaging of galaxy
clusters in the
early universe to mapping areas of
star formation in our own Galaxy.
«These findings may be telling us something very deep about the formation of
star clusters and black holes in the
early universe,» says Roeland Van Der Marel of the Space Telescope Science Institute in Baltimore.