Applying this method to one recently discovered
dwarf galaxy called Eridanus II, the scientists found a lot less dark matter in the center than many other models would have shown.
A dwarf galaxy called NGC 4625, located about 30 million light - years away in the constellation of Canes Venatici (The Hunting Dogs)
A dwarf galaxy called NGC 4625, located about 30 million light - years away in the constellation of Canes Venatici (The Hunting Dogs)(Credit: ESA / Hubble / NASA)
Researchers from the Niels Bohr Institute, among others, have detected a stream of stars in one of the Andromeda Galaxy's outer satellite galaxies,
a dwarf galaxy called Andromeda II.
The supernova, known as SN1987A, was first seen by observers in the Southern Hemisphere in 1987 when a giant star suddenly exploded at the edge of a nearby
dwarf galaxy called the Large Magellanic Cloud.
Not exact matches
The newcomer,
called Kks3, is a tiny, isolated
dwarf galaxy that sits almost 7 million light - years away in the constellation Hydrus.
These are so -
called «ultra-faint
dwarf galaxies.»
Ultra-compact
dwarfs, highlighted here within the so -
called Fornax
galaxy cluster, are a type of small star system.
They realized it must be leftovers from a pulverized
dwarf galaxy, which they
called the Sagittarius
dwarf.
The Milky Way is surrounded by 23 so -
called dwarf galaxies that are the least luminous
galaxies known.
Those remnants, which McConnachie
calls «the partially digested remains of these
dwarf galaxies,» take the form of large, diffuse streams of stars, former galactic groupings that have been pulled apart by the larger
galaxy's gravitational pull.
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.
However, most stars in the
galaxy, around 75 %, are lower mass stars
called red
dwarfs, or M stars (See Figure 1).
The
dwarf galaxy where this occurred is
called Reticulum II.
But contained within these dead stars,
called white
dwarfs, is the early history of our
galaxy, providing clues on how it came to be.
One long - standing astrophysical puzzle is that of so -
called «missing»
dwarf galaxies: the number of small
dwarf galaxies that we observe is far fewer than that predicted by theory.
Some astronomers believe brown
dwarfs may exist in large numbers, helping account for the so -
called missing mass» of galaxiesmatter
galaxies seem to contain that can not be accounted for by observed celestial objects.