This discovery is momentous
because dwarf galaxies like the LMC tend to have a lower abundance of the heavy elements that make up complex organic molecules — most importantly, oxygen, carbon, and nitrogen.
Because dwarf galaxies contain so few stars, this suggests that whatever is responsible for FRB 121102 has a better chance of forming in tiny galaxies than large, spiral ones.
Because dwarf galaxies do not host other gamma ray sources, they make ideal laboratories to search for signs of dark matter annihilation.
Not exact matches
Newberg adds that physicists hunting for particles of dark matter wafting through the Milky Way might detect fragments of Sagittarius,
because many astronomers suspect that
dwarf galaxies are especially rich in dark matter.
The standard cosmological model has told us that,
because of dark matter, there should be many more
dwarf galaxies out there, surrounding our own Milky Way, than we have found.
«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.
FRBs are probably not directly related to long gamma ray bursts (another type of explosive event that preferentially occurs in
dwarf galaxies),
because there are just too few gamma ray bursts and too many FRBs.
«
Because red
dwarfs themselves are so common,» Johnson says, «the whole
galaxy must be just swarming with little habitable planets around faint red
dwarfs.»
The stars of
dwarf galaxy Segue 1 (circled in green) are a boon to stellar archaeologists
because they're all extremely old second - generation stars.
Residing in the
dwarf galaxy IC 10, 1.8 million light - years away in the constellation Cassiopeia, the new black hole puzzles researchers
because it is thought that the kind of star that would give birth to it would not have retained enough mass to produce such a large object.
NGC 6822, about 1.6 million light - years away, is classified as an irregular
dwarf galaxy because of its odd shape and relatively small size compared with other
galaxies, such as our own, the Milky Way, and its other neighbors, the Andromeda and Triangulum
galaxies.
Because they lie much farther away and contain much less total dark matter than the center of the Milky Way,
dwarf galaxies produce a much weaker signal and require many years of observations to establish a secure detection.
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.
He suggests that the missing
dwarf galaxies could be out there but are invisible
because they are made solely of dark matter.
These flare stars are actually common
because red
dwarfs make up more than half of all starss in our
galaxy.
The discovery is a notable one
because scientists are questioning how many similar
dwarf galaxies have gone unnoticed thus far.
Because the low surface brightness
dwarf galaxies are extremely diffuse, stargazers residing in one of these
galaxies would see a night sky very different from that seen from Earth.
Yet this theory is less popular, said Metzger,
because AGNs usually exist in bigger
galaxies, not
dwarfs.
«
Dwarf galaxies like the LMC probably retained this same youthful makeup
because of their relatively low masses, which severely throttles back the pace of star formation.»
Because of the extreme intrinsic luminosity of M54 in comparison to the other globular clusters associated with SagDEG, it has been speculated early that M54 may be the nucleus of this
dwarf galaxy, or the remnant of its nucleus (Bassino and Muzzio, 1995).