Combining almost opposite ends of the electromagnetic spectrum, this
composite of the Herschel in far-infrared and XMM-Newton’s X-ray images
shows how the hot young stars detected by the X-ray observations are
sculpting and interacting with the surrounding ultra-cool gas and dust,
which, at only a few degrees above absolute zero, is the critical
material for star formation itself. Both wavelengths would be blocked by
Earth’s atmosphere, so are critical to our understanding of the
lifecycle of stars
Image Credit: ESA/Herschel/PACS/SPIRE/Hill, Motte, HOBYS Key Programme Consortium
Image Credit: ESA/Herschel/PACS/SPIRE/Hill, Motte, HOBYS Key Programme Consortium

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