| NGC
3603 is a bustling region of star birth in the Carina spiral arm of the
Milky Way galaxy, about 20,000 light years from Earth. For the first time,
this Chandra image resolves the multitude of individual X-ray sources in
this star-forming region. (The intensity of the X-rays observed by Chandra
are depicted by the various colors in this image. Green represents lower
intensity sources, while purple and red indicate increasing X-ray intensity.)
Specifically, the Chandra image reveals dozens of extremely massive stars
born in a burst of star formation about two million years ago. |
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This
region's activities may be indicative of what is happening in other distant
"starburst" galaxies (bright galaxies flush with new stars). In
the case of NGC 3603, scientists now believe that these X rays are emitted
from massive stars and stellar winds, since the stars are too young to have
produced supernovae or have evolved into neutron stars. The Chandra observations
of NGC 3603 may provide new clues about X-ray emission in starburst galaxies
as well as star formation itself. |
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