An Early Galaxy's Surprising Magnetism

Larry O'Hanlon, Discovery News
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Galaxy DLA-3C286
Galaxy DLA-3C286 | Video: Discovery Space
 

Oct. 1, 2008 -- If there had been a gargantuan refrigerator in the early universe, it might have been plastered with little magnetic galaxies. That's because the first direct measurement of an early galaxy's magnetic field has surprised astronomers by revealing a field 10 to 15 times stronger than that of our own Milky Way galaxy.

"It's enormous," said Arthur Wolfe, of San Diego's Center for Astrophysics and Space Sciences and a professor of physics at the University of California. "That was a big shock."

What makes it a surprise is that early galaxies have been thought of as hot beds of star formation. But strong galactic magnetic fields -- which are generated by cool gases that would normally coalesce to form stars -- tend to push matter apart and stave off the birth of stars.

"The theory is that it should be weaker, not stronger," Wolfe told Discovery News. Wolfe is the lead author of a paper on the discovery appearing in the Oct. 2 issue of the journal Nature.

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The very young "proto-galaxy" in question, known as DLA-3C286, is 6.5 billion light-years away, which means the radio waves collected for the study are just as old. The galaxy was chosen for the research because its radio band emissions, a form of light, have a very strong and distinct dead zone, or "absorption line," at the wavelength of 21 cm -- which is the fingerprint of hydrogen gas.

By aiming the Robert C. Byrd Green Bank Telescope at the young galaxy and applying a new technique, the team was able to detect a split in that hydrogen line which matches the effect of a strong magnetic field on hydrogen gas.


 
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