For decades astronomers have used computer models to predict
how these dwarf galaxies should orbit large galaxies.
It had been a mystery
how some dwarf galaxies can be so devoid of stars, while remaining full of dark matter.
Not exact matches
As Wetzel explained: «By improving
how we modeled the physics of stars, this new simulation offered a clear theoretical demonstration that we can, indeed, understand the
dwarf galaxies we've observed around the Milky Way.
«This mass range gets interesting, because these «ultra-faint»
dwarf galaxies are so faint that we do not yet have a complete observational census of
how many exist around the Milky Way.
Stuart Clark describes
how a superfluid Bose - Einstein state of dark matter particles might explain the streams of
dwarf satellite
galaxies in polar orbit around the Milky Way and Andromeda
galaxies (2 April, p 30).
That may mean that there's another way to create this kind of isolated
dwarf galaxy — and it could offer clues to
how galaxies in the universe form.
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.
This rare opportunity to observe a
dwarf galaxy as its gas is removed by the effects of a nearby giant
galaxy will allow scientists to learn more about
how this process happens.
The discovery is a notable one because scientists are questioning
how many similar
dwarf galaxies have gone unnoticed thus far.
Their merger into large
galaxies, therefore, could explain
how fresh material is available for the formation of G -
dwarf stars.
But contained within these dead stars, called white
dwarfs, is the early history of our
galaxy, providing clues on
how it came to be.
If we could find other systems that look like the LMC — SMC — Milky - Way system, we might be able to learn more about pairs of
dwarf galaxies and
how they interact near the halos of large
galaxies like the Milky Way.
By comparing Hubble's observations with those from the Spitzer Space Telescope the CLASH team was able to rule out red stars, brown
dwarfs, and red
galaxies as alternative explanations and concluded that the three images were a match for
how the object would appear through the gravitational lens.