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Europe's Quest for the Universe - Laboratoires de Recherche

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Development of European Astronomy 23<br />

The sou<strong>the</strong>rn Milky Way and <strong>the</strong> Magellanic Clouds (photo: C. Madsen). Just un<strong>de</strong>r<br />

<strong>the</strong> Small Magellanic Cloud is <strong>the</strong> second brightest globular cluster 47 Tucanae, just<br />

above <strong>the</strong> bar of <strong>the</strong> Large Cloud <strong>the</strong> Tarantula Nebula, a region of <strong>de</strong>nse gas and<br />

intense star <strong>for</strong>mation. The dark area in <strong>the</strong> Milky Way is <strong>the</strong> “Coal Sack” due to a<br />

nearby cloud of dust which blots out <strong>the</strong> stars behind it; at its top is <strong>the</strong> star α Crucis,<br />

which with <strong>the</strong> three bright stars to <strong>the</strong> left constitutes <strong>the</strong> “Sou<strong>the</strong>rn Cross”. The two<br />

bright stars below <strong>the</strong> Coal Sack are α and β Centauri. Just outsi<strong>de</strong> this image to <strong>the</strong><br />

left are ω Centauri, <strong>the</strong> brightest globular cluster in <strong>the</strong> sky, and Centaurus A, <strong>the</strong><br />

nearest radio galaxy (Fig. IX, 1).

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