«Not only will we learn about the formation of the black holes, but these new data from Hubble help us connect globular clusters to galaxies, providing information on one of the most important unsolved problems in astronomy today:
how galaxy structure forms in the universe,» adds Michael Rich of the University of California, Los Angeles (UCLA).
Not exact matches
Simulations of
how large - scale cosmic
structures form suggest that
galaxies are connected by a vast network of dark matter, the evasive substance that makes up most of the universe's matter but interacts with regular matter only via gravity (SN Online: 10/11/17).
Minchin views this dark
galaxy not as an anomaly but as perhaps a crucially important piece of evidence confirming current theories about
how orderly
structures — including bright
galaxies like our own — emerged from the formlessness of the Big Bang.
Astronomers would dearly have liked to get a glimpse of such
structures to find out more about
how galaxies were born.
This small stellar gathering gives astronomers clues about
how these stars form and evolve — as well as giving hints about the
structure of our
galaxy's pinwheeling arms.
«For the first time, we are not only visualizing the detailed
structure of our Local Supercluster of
galaxies but we are seeing
how the
structure developed over the history of the universe.
Several ground - based microwave telescopes, such as the South Pole Telescope, are tracking
how the
structure of very distant
galaxy clusters grew in the early Universe under the influence of gravity.
Specifically, they found that the value of the fine -
structure constant — which determines
how the
galaxies» light should appear — is one thousandth of a percent bigger today than it was 10 billion years ago.
Supercomputer simulations model
how galaxies and galactic clusters grow in long filamentary
structures known as the cosmic web.
«This goes a long way toward showing that many of our ideas of
how galaxies form and
how structures form over the history of the universe are pretty much correct,» he says.
Simulations of
how cosmic
structures form suggest that most
galaxies clump along dense filaments of dark matter, which are separated by vast cosmic voids.
The dwarf
galaxy also is of interest because it provides clues to
how the early simple universe became re-ionized by early star formation, moving it from the so - called cosmic Dark Ages of neutral gases to the development of the complexly
structured universe now in existence, where the gas between
galaxies is ionized.
Our research program started with
galaxies: Why are there so many different types, what are their histories, and
how did we get the
structures we see today — spiral, elliptical, and so forth?
The survey's researchers analyzed light from 26 million
galaxies to study
how structures in the universe have changed over the past 7 billion years — half the age of the universe.
More than that, the 3D clustering of the
galaxies lets us calculate the gravitational field between them, testing
how cosmic
structure grew over time.
«This newly discovered analogy has the potential to be a significant step forward in our understanding of turbulent flows in free - surface vortices and to provide insights into diverse areas of study ranging from civil engineering hydraulic
structures to weather systems in the atmosphere and even extending to the details of
how galaxies rotate around the black holes at their centres,» Dr Richard Sherlock, a lecturer in Physics at IT Sligo, said.
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.
«If we can measure
how much oxygen is in a
galaxy, it will tell us about all these processes,» said Shapley, who, along with Sanders, is interested in learning
how galaxies form and evolve, why
galaxies have different
structures, and
how galaxies exchange material with their intergalactic environments.
How did those modest
galaxies grow into the magnificent
structures we see around us today?
«It is remarkable
how the environment on the enormous cosmic scales seen in the dark matter
structures can influence the properties of individual stars and
galaxies - both the maturity of the stellar populations and the progressive «downsizing» of star formation to smaller
galaxies is clearly dependent on the dark matter environment,» said Scoville.
The new maps of dark matter and
galaxies will provide critical observational underpinnings to future theories for
how structure formed in the evolving universe under the relentless pull of gravity.
She explains: «I am mostly interested in
how structure forms and
how galaxies form, and
how we can use that knowledge to understand the «dark side» of the Universe...
how what we see in telescopes is connected to the dark matter of the Universe.»