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Version française
Strasbourg, the 4th of November 2003
Astronomers find nearest galaxy to the Milky Way
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(Click on image to enlarge) | An international team of astronomers from France, Italy, the UK and
Australia has found a previously unknown galaxy colliding with our own
Milky Way. This newly-discovered galaxy takes the record for the
nearest galaxy to the centre of the Milky Way. Called the Canis Major
dwarf galaxy after the constellation in which it lies, it is about
25000 light years away from the solar system and 42000 light years
from the centre of the Milky Way. This is closer than the Sagittarius
dwarf galaxy, discovered in 1994, which is also colliding with the
Milky Way. The discovery shows that the Milky Way is building up its
own disk by absorbing small satellite galaxies. The research is to be
published in the Monthly Notices of the Royal Astronomical Society
within the next few weeks.
The discovery of the Canis Major dwarf was made possible by a recent
survey of the sky in infrared light (the Two-Micron All Sky Survey or
"2MASS"), which has allowed astronomers to look beyond the clouds of
dust in the disk of the Milky Way. Until now, the dwarf galaxy lay
undetected behind the dense disk. "It's like putting on infrared night
vision goggles," says team-member Dr Rodrigo Ibata of Strasbourg
Observatory. "We are now able to study a part of the Milky Way that
has been previously out of sight".
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(Click on image to enlarge) | The new dwarf galaxy was detected by its M-giant stars -- cool, red
stars that shine especially brightly in infrared light. "We have used
these rare M-giant stars as beacons to trace out the shape and
location of the new galaxy because its numerous other stars are too
faint for us to see," explains Nicolas Martin, also of Strasbourg
Observatory. "They are particularly useful stars as we can measure
their distances, and so map out the three-dimensional structure of
distant regions of the Milky Way disk." In this way, the astronomers
found the main dismembered corpse of the dwarf galaxy in Canis Major
and long trails of stars leading back to it. It seems that streams of
stars pulled out of the cannibalised Canis Major galaxy not only
contribute to the outer reaches of the Milky Way's disk, but may also
pass close to the Sun.
Astronomers currently believe that large galaxies like the Milky Way
grew to their present majestic proportions by consuming their smaller
galactic neighbours. These cannibalised galaxies add stars to the vast
haloes around large galaxies. However, until now, they did not
appreciate that even the disks of galaxies can grow in this
fashion. Computer simulations show that the Milky Way has been taking
stars from the Canis Major dwarf and adding them to its own disk - and
will continue to do so.
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(Click on image to enlarge) |
"On galactic scales, the Canis Major dwarf galaxy is a lightweight of
about only one billion Suns," said Dr. Michele Bellazzini of Bologna
Observatory. "This small galaxy is unlikely to hold together much
longer. It is being pushed and pulled by the colossal gravity of our
Milky Way, which has been progressively stealing its stars and pulling
it apart." Some remnants of the Canis Major dwarf form a ring around
the disk of the Milky Way.
"The Canis Major dwarf galaxy may have added up to 1% more mass to our
Galaxy," said Dr Geraint Lewis of the University of Sydney. "This is
also an important discovery because it highlights that the Milky Way
is not in its middle age - it is still forming." "Past interactions of
the sort we are seeing here could be responsible for some of the
exquisite detail we see today in the structure of the Galaxy," says Dr
Michael Irwin of the University of Cambridge.
Animations
Journey to the Canis Major galaxy (mpeg)
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Evolution of the Canis Major galaxy orbiting the Milky Way for 2 billion years (mpeg)
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Contact information:
- Dr Rodrigo Ibata, Observatoire de Strasbourg - France (Tel : +33 (0)3 90 24 23 91)
- Nicolas Martin, Observatoire de Strasbour - France (Tel : +33 (0)3 90 24 24 88)
- Dr Geraint Lewis, School of Physics, University of Sydney - Australia (Tel : +61 2 9351 5184)
- Dr Michael Irwin, Institute of Astronomy, Cambridge - United Kingdom (Tel : +44 (0)1223 337524)
- Dr Michele Bellazzini, INAF - Osservatorio Astronomico di Bologna - Italy (Tel : +39 051 20 95 773)
- Dr Walter Dehnen, University of Leiceister - United Kingdom (Tel : +44 (0)116 2523549)
Press contacts
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