Not exact matches
«When more - powerful detectors provide us with more observations,» Mészáros said, «we also will be able to use Fast Radio Bursts as a probe of their host galaxies, of the space between galaxies, of the
cosmic -
web structure of the universe, and as a test of fundamental physics.»
Spinning the
Cosmic Web The first inkling of the gaping holes in the universe's distribution of galaxies came in the late 1970s, when astronomers began sketching out the three - dimensional
structure of the cosmos.
The scaffolding that holds the large - scale
structure of the universe constitutes galaxies, dark matter and gas (from which stars are forming), organized in complex networks known as the
cosmic web.
[1] The
cosmic web is the
structure of the Universe at the largest scale.
The location of galaxies or clusters in this enormous
cosmic web tests our understanding of the way
structure forms in the universe.
The gaseous components of this
web are normally extremely difficult to detect, so the illuminated halos of gas surrounding the quasars deliver an almost unique opportunity to study the gas within this large - scale
cosmic structure.
The team has also found that the rotation axes of these quasars tend to be aligned with the vast
structures in the
cosmic web in which they reside.
Supercomputer simulations model how galaxies and galactic clusters grow in long filamentary
structures known as the
cosmic web.
«From the distribution of galaxies we can infer where the filaments of the
cosmic web are, and the nebula is perfectly aligned with that
structure,» he said.
The MAMMOTH - 1 nebula appears to have a filamentary
structure that aligns with the galaxy distribution in the large - scale
structure of the protocluster, supporting the idea that ELANs are illuminated segments of the
cosmic web, Cai said.
The standard cosmological model of
structure formation in the universe predicts that galaxies are embedded in a
cosmic web of matter, most of which is invisible dark matter.
The newly defined
cosmic velocity
web defines the
structure of the universe from velocity information alone.
Filament
structures in the
cosmic web are shown at different time periods, ranging from when the universe was 12.3 billion years old (left) to when the universe was 7.4 billion years old (right).
(VIDEO) Visualizing the
cosmic web: This computerized simulation by the Virgo Consortium, called the Millennium Simulation, shows a
web - like
structure in the universe composed of galaxies and the dark matter around them.
The map provides a tantalizing glimpse of giant filamentary
structures extending across millions of light - years, and paves the way for more extensive studies that will reveal not only the
structure of the
cosmic web, but also details of its function — the ways that pristine gas is funneled along the
web into galaxies, providing the raw material for the formation of galaxies, stars, and planets.
Combining all of the measurements across the entire field of view allowed the team a tantalizing glimpse of giant filamentary
structures extending across millions of light - years, and paves the way for more extensive studies that will reveal not only the
structure of the
cosmic web, but also details of its function — the ways that pristine gas is funneled along the
web into galaxies, providing the raw material for the formation of galaxies, stars, and planets.
This map, built from data collected from the W. M. Keck Observatory, is millions of light - years across and provides a tantalizing glimpse of large
structures in the «
cosmic web» — the backbone of
cosmic structure.
Theories, computer models, and indirect observations have indicated that there is a
cosmic web of dark matter that connects galaxies and constitutes the large - scale
structure of the cosmos.
This would show the
structure of the so - called «
cosmic web» that galaxies are embedded inside, and how chemically enriched gases flow in and out of a galaxy to fuel star formation.
Hubble's spectrographs — partially fulfilling the promise of a large space telescope envisioned by Spitzer all those years ago — were critical in allowing astronomers to map the
web - like
structure of intergalactic gas in the universe, now termed the «
cosmic web.»
Since these filaments do not emit any light of their own, the astronomers studied their
structure and composition by analyzing light from distant quasars as it passed through the
cosmic web.