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Martin Pugh

NGC 6188 - Emission Nebula in Ara

New 4 frame High-Resolution Mosaic - Apr-Jun 2007

                          

Image Capture and Processing Details - Click Here

 

                    
 

The left hand image was processed by myself before I passed the data to Rob Gendler.
His far superior version is shown at right. 
 

NGC 6188 is an interstellar carnival of young blue stars, hot red gas, and cool dark dust. Located 4000 light years away in the disk of our Galaxy, NGC 6188 is home to the Ara OB1 association, a group of bright young stars whose nucleus forms the open cluster NGC 6193. These stars are so bright that some of their blue light reflects off of interstellar dust forming the diffuse blue glow in the top left hand quadrant of the image above. NGC 6193 formed about three million years ago from the surrounding gas, and appears unusually rich in close binary stars. The red glow visible throughout the photograph arises from hydrogen gas heated by the bright stars in Ara OB1. The dark dust that blocks much of NGC 6188's light was likely formed in the outer atmospheres of cooler stars and in supernovae ejecta.

 

(Text taken from http://antwrp.gsfc.nasa.gov/apod/ap990825.html)

                                       

                                                           

                                                              HA only version


 

 3315 x 2335
     (50%)

4973 x 3487
     (75%)                              

 
 

Equipment

Telescope:                Takahashi FS128 @ f6
Mount:                      Paramount ME by Software Bisque
Instrument:               STL11000M CCD Camera by SBIG

Exposure:                  This is an (HA+R)RGB Image of exposures 300:150:150:150
Capture Software:       CCDSOFT V5 and CCD AutoPilot
Processing:                Maxim DL/CCD, Photoshop CS2

Telescope:              12.5" RCOS by RC Optical Systems @f9.1
Mount:                      Paramount ME by Software Bisque
Instrument:               STL11000M CCD Camera by SBIG with AO-L

Exposure:                  4 Frame Mosaic - Each Frame LRGB 240:60:60:60 minutes.  Plus a central
                                "Patch" Lum frame of 180 minutes.
Capture Software:       CCDSOFT V5 and CCD AutoPilot V3.4
Processing:                Maxim DL/CCD, Photoshop CS2, CCDStack.

 

 

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