One of the rare and brief bursts of cosmic radio waves that have puzzled astronomers since they were first detected nearly 10 years ago has finally been tied to a source: an older
dwarf galaxy more than 3 billion light years from Earth.
Not exact matches
The Small Magellanic Cloud (SMC) is a
dwarf galaxy, the
more petite twin of the Large Magellanic Cloud (LMC).
[Sukanya Chakrabarti et al, Clustered Cepheid Variables 90 kiloparsec from the Galactic Center]
Dwarf galaxies like this one are thought to contain
more dark matter than regular matter.
A
dwarf galaxy near the Milky Way may consist of
more dark matter than regular matter.
The small red circles denote other objects that emit X-rays, like neutron stars or white
dwarfs, that are found scattered around
more of the
galaxy.
Images of M32, a
dwarf elliptical
galaxy near to our own, show that stars become clustered much
more closely together near its centre, which is what should happen if the
galaxy contains a black hole.
Astronomers studying a nearby
dwarf galaxy have detected large organic molecules, suggesting that the basic chemical building blocks of life can form in places much
more primitive than our own
galaxy.
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.
As observation techniques have improved,
more dwarf galaxies have been spotted orbiting the Milky Way.
«Dark Energy Survey finds
more celestial neighbors: New
dwarf galaxy candidates could mean our sky is
more crowded than we thought.»
Astronomers have developed a number of theories for why we haven't found
more, but none of them could account for both the paucity of
dwarf galaxies and their properties, including their mass, size, and density.
Despite having run the highest - resolution simulation to date, Wetzel continues to push forward, and he is in the process of running an even higher - resolution,
more - sophisticated simulation that will allow him to model the very faintest
dwarf galaxies around the Milky Way.
«Just this year,
more than 20 of these
dwarf satellite
galaxy candidates have been spotted, with 17 of those found in Dark Energy Survey data,» said Alex Drlica - Wagner of the U.S. Department of Energy's (DOE) Fermi National Accelerator Laboratory, one of the leaders of the DES analysis.
Further tests are ongoing, and data collected during the second year of the Dark Energy Survey could yield
more of these potential
dwarf galaxies to study.
Known as an ultra-compact
dwarf, this type of system has up to a billion stars and can be similar in mass to a
galaxy, but it is compact and looks
more like a star cluster.
Scientists took measurements to see what was happening inside the
galaxies, and something didn't add up; the ultra-compact
dwarf galaxies had
more mass than their stars alone could account for.
Two of them — a
more extensive survey of luminous
galaxies, intended to tease out
more information about
galaxy clustering on large scales, and a
more sensitive search for the cannibalized remnants of
dwarf galaxies — will extend recent findings from the second Sloan survey.
In our
galaxy, newborn stars span an enormous range of masses: A few rare superstars arise with
more than 100 times the mass of our sun, but the vast majority is composed of dim red
dwarfs with just a fraction of the sun's mass.
Fast radio bursts are brief, bright pulses of radio emission from distant but so far unknown sources, and FRB 121102 is the only one known to repeat:
more than 200 high - energy bursts have been observed coming from this source, which is located in a
dwarf galaxy about 3 billion light years from Earth.
The team located the FRB about 100,000 times
more precisely than previous attempts with individual telescopes, letting them unambiguously associate it with a
dwarf galaxy about a tenth of the diameter of the Milky Way,
more than 2.5 billion light years away (Nature, doi.org/bwss).
Previous observations of superluminous supernovae found they typically reside in low - mass or
dwarf galaxies, which tend to be less enriched in metals than
more massive
galaxies.
If all such compact
dwarf galaxies are stripped, she argues, then their black holes may also be unexpectedly massive — meaning these behemoths are much
more abundant in the universe than previously thought.
Simulations of cold dark matter predict tens to hundreds of times
more dwarf galaxies than anyone can find.
The Gemini observations also determined that the
dwarf galaxy is
more than 3 billion light - years from Earth.
Through its detailed pictures, Keck allows us to learn
more about puny brown
dwarfs, raging weather on Jupiter, super dense
galaxies and other celestial happenings.
Some
galaxies like our own are predicted to have about 30 times
more dark matter than normal matter, whereas
dwarf galaxies can have up to 400 times
more.
The densest places would have had
more rapid star formation to make the elliptical
galaxies while the lower density concentrations would have made the spiral
galaxies and
dwarf galaxies.
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.
There may be
more irregular and
dwarf galaxies.
The Canis Major
Dwarf galaxy about 25,000 light years from us is in a
more advanced stage of «digestion» by the Milky Way — just the nucleus of a former
galaxy is all that is left.
These flare stars are actually common because red
dwarfs make up
more than half of all starss in our
galaxy.
We also needed to add in the contribution of a
more abundant population of faint
dwarf galaxies,» lead author Hakim Atek, from the Ecole Polytechnique Fédérale de Lausanne, said in a statement.
The big bang, black holes, dark matter, dark energy, extrasolar planets, brown
dwarfs, quasars, pulsars, cosmic rays, the space - time continuum,
galaxies and
more galaxies.
More than 20
dwarf galaxy companions have been discovered in the past year, many of which were also discovered with DECam.
They hope to localize
more bursts to see whether they usually live in
dwarf irregular
galaxies, and whether they all appear alongside steady radio sources, both of which would support the newborn - magnetar theory.
Were they
more recently captured as an already - merging pair of
dwarf galaxies?
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.
While theory and observations agree for
galaxies with circular velocities above ~ 100 km / s, theory predicts far
more dwarfs below this velocity than we observe.
In 2003, astronomers announced that they had discovered that iron from supernovae of the first stars (possibly from Type Ia supernovae involving white
dwarfs) indicate that «massive chemically enriched
galaxies formed» within one billion years after the Big Bang, and so the first stars may have preceded the birth of supermassive black holes (
more from Astronomy Picture of the Day, ESA, and Freudling et al, 2003).
These signatures tells us that the external regions of the stellar halo might contain the remains of one, or
more, massive
dwarf galaxy, devoured by the Milky Way.
Two super-Earths have been detected around Kapteyn's Star (an orphan star torn from an ancient
dwarf satellite
galaxy of the Milky Way), one within its habitable zone (
more).