2014 February 1
NGC 6188 and NGC 6164
Image Credit & Copyright: Harel Boren and Tal Faibish
Explanation: Fantastic shapes lurk in clouds of glowing gas in NGC 6188, about 4,000 light-years away. The
emission nebula is found near the edge of a large molecular cloud unseen at visible wavelengths, in the southern
constellation Ara. Massive, young
stars of the embedded Ara
OB1 association were formed in that region only a few million years ago,
sculpting the dark shapes and powering the nebular glow with stellar winds and intense ultraviolet radiation. The recent
star formation itself was likely triggered by winds and supernova explosions, from previous generations of massive stars, that swept up and compressed the molecular gas. Joining NGC 6188 on this cosmic canvas is rare emission nebula
NGC 6164, also created by one of the region's massive O-type stars. Similar in appearance to many
planetary nebulae, NGC 6164's striking, symmetric gaseous shroud and faint halo surround its bright central star near the bottom edge. The impressively
wide field of view spans over 3 degrees (six full Moons), corresponding to over 200 light years at the estimated distance
of NGC 6188. Narrowband image data has been included in
the natural looking color composite, adding to deep red emission from hydrogen and sulfur atoms and the blue-green light of oxygen atoms.
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