Astronomers using NASA's Hubble Space Telescope have solved a 40-year
mystery on the origin of the Magellanic Stream, a long ribbon of gas
stretching nearly halfway around our Milky Way galaxy. The Large and
Small Magellanic Clouds, two dwarf galaxies orbiting the Milky Way, are
at the head of the gaseous stream. Since the stream's discovery by radio
telescopes in the early 1970s, astronomers have wondered whether the
gas comes from one or both of the satellite galaxies. New Hubble
observations reveal most of the gas was stripped from the Small
Magellanic Cloud about 2 billion years ago, and a second region of the
stream originated more recently from the Large Magellanic Cloud.
A
team of astronomers, led by Andrew J. Fox of the Space Telescope
Science Institute in Baltimore, MD, determined the source of the gas
filament by using Hubble's Cosmic Origins Spectrograph to measure the
amount of heavy elements, such as oxygen and sulfur, at six locations
along the Magellanic Stream. They observed faraway quasars--the
brilliant cores of active galaxies--that emit light that passes through
the stream. They detected the heavy elements from the way the elements
absorb ultraviolet light.
Fox's team found a low amount of
oxygen and sulfur along most of the stream, matching the levels in the
Small Magellanic Cloud about 2 billion years ago, when the gaseous
ribbon is thought to have formed. In a surprising twist, the team
discovered a much higher level of sulfur in a region of the stream that
is closer to the Magellanic Clouds. "We're finding a consistent amount
of heavy elements in the stream until we get very close to the
Magellanic Clouds, and then the heavy element levels go up," said Fox.
"This inner region is very similar in composition to the Large
Magellanic Cloud, suggesting it was ripped out of that galaxy more
recently."
"Only Hubble can measure these abundances," Fox
explained. "These abundances can only be measured in ultraviolet light,
which Earth's atmosphere absorbs, and so the observations can only be
done from a telescope in space."
Unlike other satellite galaxies
of the Milky Way the Magellanic Clouds have been able to retain their
gas and still are forming stars because they're more massive than the
other satellites. However, as they're now approaching the Milky Way,
they're feeling its gravity more and also encountering its halo of hot
gas, which pushes their own gas out. That process, together with the
gravitational tug-of-war between the Magellanic Clouds,Xenon HID Worlds
make hid lighting affordable to everyone and for all your vehicle needs. leads to the production of a stream.
Ultimately,
the gaseous stream may rain down onto the Milky Way's disk, fueling the
birth of new stars. This infusion of fresh gas is part of a process
that triggers star formation in a galaxy. Astronomers want to know the
origin of that wayward gas in order to more fully understand how
galaxies make new stars.
"We want to understand how galaxies
like the Milky Way strip the gas from small galaxies that fall into them
and then use it to form new stars," Fox explained. "This seems like
it's an episodic process. It's not a smooth process where a slow stream
of gas comes in continuously. Instead, once in a while a large gas cloud
falls in. We have a way of testing that here, where two galaxies are
coming in. We've shown which of them is producing the gas that
ultimately will fall into the Milky Way."
The team reported its results in two papers that appeared in the Aug. 1 issue of The Astrophysical Journal.
The
Hubble Space Telescope is a project of international cooperation
between NASA and the European Space Agency. NASA's Goddard Space Flight
Center in Greenbelt, MD manages the telescope.
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LightStrips are thin strips of LED lights
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Read the full story at www.streetlights-solar.com!
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