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HST and Chandra Composite of NGC 604
Credit: NASA/CXC/CfA/R. Tuellmann et al.; Optical: NASA/AURA/ STScI


Evacuation Route

The beautiful image above of the star cluster NGC 604 in the nearby galaxy M33 is a combination of a high-resolution image by the Hubble Space Telescope plus an X-ray image by the Chandra X-ray Observatory. This image is one of the best ever obtained showing the interaction of stars and their environment. The Hubble image shows how the massive stars have formed together, and how their combined winds (and the explosive deaths of the most massive members?) have carved out huge bubbles, which (as the Chandra image, in blue, shows) are filled with hot shocked gas. The Chandra X-ray image suggests that most of the hot gas was produced by a combination of stellar winds on the right side of the cluster. However, on the left side of the cluster, the bright X-ray emission does not appear to be associated with stars, so that supernovae probably played a more important role in producing the hot X-ray emitting gas. The HST and Chandra data implies that a massive wall of gas shields the relatively quiet region on the left from the active star formation on the right.
Published: February 02, 2009


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Page Author: Dr. Michael F. Corcoran
Last modified Friday, 20-Apr-2012 15:25:30 EDT