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Life and Death in a Star-Forming Cloud (Herschel)
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 More options Nov 14 2012, 3:01 pm
Newsgroups: sci.space.news
Followup-To: sci.space.policy
From: baa...@earthlink.net
Date: Wed, 14 Nov 2012 19:51:14 +0000 (UTC)
Local: Wed, Nov 14 2012 2:51 pm
Subject: Life and Death in a Star-Forming Cloud (Herschel)

http://www.jpl.nasa.gov/news/news.php?release=2012-358  

Life and Death in a Star-Forming Cloud
Jet Propulsion Laboratory
November 14, 2012

The aftershock of a stellar explosion rippling through space is captured
in this new view of the supernova remnant called W44. The image combines
longer-wavelength infrared and X-ray light captured by the European
Space Agency's Herschel and XMM-Newton space observatories.

NASA also plays an important role in the Herschel mission, with the U.S
project office based at the agency's Jet Propulsion Laboratory in
Pasadena, Calif.

W44 is located about 10,000 light-years away, within a forest of dense
star-forming clouds in the constellation of Aquila, the Eagle. It is one
of the best examples of a supernova remnant interacting with its parent
cloud.

The supernova remnant is the result of a massive star that reached the
end of its life and expelled its outer layers in a dramatic explosion.
All that remains of the stellar behemoth is the spinning core of a
neutron star, or pulsar.

Identified as PSR B1853+01, the pulsar is the bright point to the top
left in W44, colored light blue in this image. It is thought to be
around 20,000 years old. Like all pulsars, as it rapidly rotates, it
sweeps out a wind of highly energetic particles and beams of light
ranging from radio to X-ray energies. The center of the supernova
remnant is also bright in X-rays, coming from the hot gas that fills the
shell at temperatures of several million degrees.

Herschel's infrared eyes seek out regions of gently heated gas and dust
farther from W44, where new stars are congregating. Examples include the
arrowhead-shaped star-formation region to the right of W44, which
appears to point to another trio of intricate clouds further to the
right and above. More broadly, a number of compact objects scattered
across the scene map the cold seeds of future stars that will eventually
emerge from their dusty cocoons. Finally, diffuse purple emission
towards the bottom left of the image provides a glimpse of the plane of
our Milky Way galaxy.

Herschel is a European Space Agency cornerstone mission, with science
instruments provided by consortia of European institutes and with
important participation by NASA. NASA's Herschel Project Office is based
at JPL, which contributed mission-enabling technology for two of
Herschel's three science instruments. The NASA Herschel Science Center,
part of the Infrared Processing and Analysis Center at the California
Institute of Technology in Pasadena, supports the United States
astronomical community. Caltech manages JPL for NASA.

More information is online at http://www.herschel.caltech.edu ,
http://www.nasa.gov/herschel and http://www.esa.int/SPECIALS/Herschel .

Whitney Clavin (818) 354-4673
Jet Propulsion Laboratory, Pasadena, Calif.
whitney.cla...@jpl.nasa.gov

2012-358


 
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