Frequent Starbursts Sterilize Center of Milky Way (Forwarded)

From: Andrew Yee (ayee_at_nova.astro.utoronto.ca)
Date: 10/14/04 

Date: Thu, 14 Oct 2004 16:13:39 -0400

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Release No.: 04-31

For Release: October 4, 2004

Frequent Starbursts Sterilize Center of Milky Way

Cambridge, MA -- Life near the center of our galaxy never had a chance. Every 20
million years on average, gas pours into the galactic center and slams together,
creating millions of new stars. The more massive stars soon go supernova,
exploding violently and blasting the surrounding space with enough energy to
sterilize it completely. This scenario is detailed by Smithsonian astronomer
Antony Stark (Harvard-Smithsonian Center for Astrophysics) and colleagues in the
October 10, 2004, issue of The Astrophysical Journal Letters.

The team's discovery was made possible using the unique capabilities of the
Antarctic Submillimeter Telescope and Remote Observatory (AST/RO). It is the
only observatory in the world able to make large-scale maps of the sky at
submillimeter wavelengths.

The gas for each starburst comes from a ring of material located about 500
light-years from the center of our galaxy. Gas collects there under the
influence of the galactic bar -- a stretched oval of stars 6,000 light-years
long rotating in the middle of the Milky Way. Tidal forces and interactions with
this bar cause the ring of gas to build up to higher and higher densities until
it reaches a critical density or "tipping point." At that point, the gas
collapses down into the galactic center and smashes together, fueling a huge
burst of star formation.

"A starburst is star formation gone wild," says Stark.

Astronomers see starbursts in many galaxies, most often colliding galaxies where
lots of gas crashes together. But starbursts can happen in isolated galaxies
too, including our own galaxy, the Milky Way.

The next starburst in the Milky Way is coming relatively soon, predicts Stark.
"It likely will happen within the next 10 million years."

That assessment is based on the team's measurements showing that the gas density
in the ring is nearing the critical density. Once that threshold is crossed, the
ring will collapse and a starburst will blaze forth on an unimaginably huge scale.

Some 30 million solar masses of matter will flood inward, overwhelming the 3
million solar mass black hole at the galactic center. The black hole, massive as
it is, will be unable to consume most of the gas.

"It would be like trying to fill a dog dish with a firehose," says Stark.
Instead, most of the gas will form millions of new stars.

The more massive stars will burn their fuel quickly, exhausting it in only a few
million years. Then, they will explode as supernovae and irradiate the
surrounding space. With so many stars packed so close together as a result of
the starburst, the entire galactic center will be impacted dramatically enough
to kill any life on an Earth-like planet. Fortunately, the Earth itself lies
about 25,000 light-years away, far enough that we are not in danger.

The facility used to make this discovery, AST/RO, is a 1.7-meter-diameter
telescope that operates in one of the most challenging environments on the
planet -- the frigid desert of Antarctica. It is located at the National Science
Foundation's Amundsen-Scott Station at the South Pole. The air at the South Pole
is very dry and cold, so radiation that would be absorbed by water vapor at
other sites can reach the ground and be detected.

"These observations have helped advance our understanding of star formation in
the Milky Way," says Stark. "We hope to continue those advancements by
collaborating with researchers who are working on the Spitzer Space Telescope's
Legacy Science Program. AST/RO's complementary observations would uniquely
contribute to that effort."

Stark's co-authors on the paper announcing this finding are Christopher L.
Martin, Wilfred M. Walsh, Kecheng Xiao and Adair P. Lane (Harvard-Smithsonian
Center for Astrophysics), and Christopher K. Walker (Steward Observatory).

Headquartered in Cambridge, Mass., the Harvard-Smithsonian Center for
Astrophysics (CfA) is a joint collaboration between the Smithsonian
Astrophysical Observatory and the Harvard College Observatory. CfA scientists,
organized into six research divisions, study the origin, evolution and ultimate
fate of the universe.

Note to Editors:

High-resolution images to accompany this release are available online at
      http://www.cfa.harvard.edu/press/pr0431image.html

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