by APOD Robot » Wed Mar 30, 2016 4:09 am
NGC 6188 and NGC 6164
Explanation: Fantastic shapes lurk in clouds of glowing gas in the giant star forming region NGC 6188. The
emission nebula is found about 4,000
light years away 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, visible toward the lower right, 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. Three image sets have been included in
the featured composite.
[/b]
[url=http://apod.nasa.gov/apod/ap160330.html][img]http://apod.nasa.gov/apod/calendar/S_160330.jpg[/img] [size=150]NGC 6188 and NGC 6164[/size][/url]
[b] Explanation: [/b] [url=http://apod.nasa.gov/apod/ap100716.html]Fantastic shapes[/url] lurk in clouds of glowing gas in the giant star forming region NGC 6188. The [url=http://fusedweb.llnl.gov/CPEP/Chart_Pages/5.Plasmas/Nebula/Emission.html]emission nebula[/url] is found about 4,000 [url=https://www.grc.nasa.gov/www/k-12/Numbers/Math/Mathematical_Thinking/how_long_is_a_light_year.htm]light years[/url] away near the edge of a large molecular cloud unseen at visible wavelengths, in the southern [url=http://en.wikipedia.org/wiki/Ara_(constellation)]constellation Ara[/url]. Massive, young [url=http://arxiv.org/abs/1105.3629]stars of[/url] the embedded Ara [url=http://en.wikipedia.org/wiki/Stellar_association#Stellar_associations]OB1 association[/url] were formed in that region only a few million years ago, [url=http://apod.nasa.gov/apod/ap080313.html]sculpting[/url] the dark shapes and powering the nebular glow with stellar winds and intense [url=http://missionscience.nasa.gov/ems/10_ultravioletwaves.html]ultraviolet radiation[/url]. The recent [url=http://archive.ncsa.uiuc.edu/Cyberia/Bima/StarForm.html]star formation[/url] itself was likely triggered by winds and supernova explosions, from previous generations of massive [url=https://www.nasa.gov/subject/6892/stars/]stars[/url], that swept up and compressed the molecular gas. Joining NGC 6188 on this cosmic canvas, visible toward the lower right, is rare emission nebula [url=http://apod.nasa.gov/apod/ap140522.html]NGC 6164[/url], also created by one of the region's massive [url=https://en.wikipedia.org/wiki/O-type_star]O-type stars[/url]. Similar in appearance to many [url=http://apod.nasa.gov/apod/ap110218.html]planetary nebulae[/url], NGC 6164's striking, symmetric gaseous shroud and faint [url=http://cdn.c.photoshelter.com/img-get/I00006OqX0jGWHmQ/s/750/750/lode00006.jpg]halo surround[/url] its bright central star near the bottom edge. The impressively [url=http://apod.nasa.gov/apod/image/1402/ngc6188_fieldlab.jpg]wide field of view[/url] spans over 3 degrees (six full Moons), corresponding to over 200 light years at the estimated distance [url=http://www.youtube.com/watch?v=Gn9mZpAcbF8]of NGC 6188[/url]. Three image sets have been included in [url=http://martinpughastrophotography.id.au/images/NGC6188_Composite.jpg]the featured composite[/url].
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