Hassled galaxy 'thriving
on chaos'

Embargoed
until 0600 AEDT Friday 11 March 2005 (1400 US Eastern Standard Time, March 10,
2005) in accordance with publication in Science.

Powerful but unknown forces are at work in a small companion galaxy of the
Milky Way, astronomers say in today’s issue of the journal Science.



Something is keeping the structure and magnetic field of this galaxy—the
Large Magellanic Cloud—strong and ordered, even while the Milky Way’s
gravity works to tear them apart.



A team led by Bryan Gaensler of the Harvard-Smithsonian Center for Astrophysics
used the CSIRO Australia Telescope near Narrabri in NSW to study the galaxy’s
magnetic field.



“This is the most detailed map ever made of another galaxy’s magnetism,”
says Gaensler.



At just 160 000 light-years away the Large Magellanic Cloud, or LMC, is the
Milky Way’s closest neighbour and is being clawed apart by the Milky Way’s
gravity. The researchers were surprised that the LMC's magnetic field is so
smooth and ordered, given the internal turmoil the galaxy must experience.



“It’s like having a birthday party all afternoon for a bunch of
4-year-olds, and then finding the house still neat and tidy when they leave,”
Gaensler says. “Some powerful forces must be at work to keep the magnetic
field from being messed up.”



The Milky Way and many other large spiral galaxies have well-organised, large-scale
magnetic fields. It’s thought that the overall rotation of these galaxies
combines and smooths out the small-scale magnetic fields created by whirls and
eddies of gas. The process is called a ‘dynamo’, and is similar
to the process that produces the Earth’s magnetic field.



“But if a galaxy experiences sudden bursts of star formation or supernova
explosions, the energy that these processes release should completely disrupt
the large-scale magnetic field,” says Lister Staveley-Smith of the CSIRO
Australia Telescope National Facility.



“And we know the LMC has had those kind of violent events over the last
several thousand million years,” he says.



So what keeps the LMC’s magnetic field in order? There are several possibilities,
the researchers say, but the process they favour is one driven by extremely
energetic particles called ‘cosmic rays’. This would take effect
more quickly than the conventional dynamo mechanism. It also requires vigorous
star formation to operate, so “stars bursting out at random all over would
strengthen the magnetic field, not mess it up,” says Gaensler. “You
could say this galaxy is thriving on chaos.”

Further information

Images

Publication

B.M. Gaensler, M. Haverkorn, L.Staveley-Smith, J.M. Dickey, N.M. McClure-Griffiths,
J.R. Dickel and M. Wolleben. “The magnetic field of the Large Magellanic
Cloud revealed through Faraday rotation.” Science, 307
(5715): 1610 (11 March 2005). PDF

 


 

Contacts

Bryan Gaensler, Harvard-Smithsonian Center for Astrophysics

+1-617-869-7153 (mob)

+1-617-496-7854 (office)

bgaensler@cfa.harvard.edu

Lister Staveley-Smith, CSIRO Australia Telescope National Facility

+61-2-9372-4271 (office)

+61-425-212-592 (mob.)

Lister.Staveley-Smith@csiro.au

(for media assistance) Helen Sim, CSIRO Australia Telescope National Facility


+61-2-9372-4251 (office)

+61-419-635-905 (mob)

Helen.Sim@csiro.au

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