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Infrarotbild der Schockwelle (roter Bogen), die von dem massereichen Riesenstern Zeta Ophiuchi in einer interstellaren Staubwolke erzeugt wird. Die schwachen Winde von sonnenähnlichen Hauptreihensternen sind viel schwieriger zu beobachten
NASA/JPL-Caltech; NASA and The Hubble Heritage Team (STScI/AURA); Acknowledgment: C. R. O'Dell, Vanderbilt University
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