jase
08-10-2011, 08:15 PM
Hi All,
Still getting through the data acquired on previous observations. I decided to shoot this region as its very close to IC4628 of which I enjoy imaging. In hindsight I should have also incorporated this area as part of the greater mosaic I produced...perhaps another time. Anyway, here is my rendition of RCW119.
>>> RCW119 (http://cosmicphotos.com/gallery/image.php?fld_image_id=240&fld_album_id=11)
Located in the constellation Scorpius is the rich HII region that is dominated by the open star cluster NGC 6281 seen at center of the presented image. The cluster has a mass of around 214 solar masses consisting of 55 stars with the brightest star being 9th magnitude. Overall, its integrated visual magnitude of 5.4 makes it easily observable with binoculars or small telescopes. The region contains various HII nebulae with the most prominent being RCW 119 (aka Sh 2-2, Gum 57) which forms a wind swept bubble caused by the eclipsing binary HD 153919. There are two other distinct nebula in the scene towards the right beyond the bubble. RCW 120 (aka Sh 2-3, Gum 58) appears as a 'S' shaped nebula with a dark nebula rift passing through it. Below this is the small, yet interesting planetary nebula known as the Bug Nebula due to its features (aka NGC 6302, Sh 2-6, Gum 60, RCW 124). The star cluster NGC 6281 resides 1,600 light years away, with most of the HII nebulosity much further in distance such as RCW 120 at 4,300 light years.
I will be honest, I had different intentions with this image. I acquired approximately 16hrs in total of Ha, OIII and SII data but found the area doesn't have a strong presence of OIII so didn't bother with a narrowband composite. I may consider working the data over just for fun, but there are other projects to move on to. The final result is noted as a HaRGB composite however I did blend a small amount of OIII into the areas where it was present in the raw master sub (done as a colour dodge blend mode). This gives the appearance of weak Ha+R blend alas it potentially a more accurate representation. I validated this with the base RGB master I use as a stars layer to confirm the areas were indeed less saturated in the red hue. I guess this all comes back down to a matter of taste but I'm fine with the result but the process need refinement. If you are wondering which star is HD 153919, its the bright one to very close to the lower left of the cluster NGC6281. The bubble/shock wave bow to the right is quite impressive. I'll try produce an annotated version when I get a chance. The Ha data set is certainly rich in detail. The bug nebula adds a cool dimension too. Not many other thoughts to add about this image. I defaulted back to MaximDL for pixel math Ha+R combine on the image as I had problems with CCDStack doing the task. Probable user error, I'll need to check it out again.
Thanks for checking it out. :)
Still getting through the data acquired on previous observations. I decided to shoot this region as its very close to IC4628 of which I enjoy imaging. In hindsight I should have also incorporated this area as part of the greater mosaic I produced...perhaps another time. Anyway, here is my rendition of RCW119.
>>> RCW119 (http://cosmicphotos.com/gallery/image.php?fld_image_id=240&fld_album_id=11)
Located in the constellation Scorpius is the rich HII region that is dominated by the open star cluster NGC 6281 seen at center of the presented image. The cluster has a mass of around 214 solar masses consisting of 55 stars with the brightest star being 9th magnitude. Overall, its integrated visual magnitude of 5.4 makes it easily observable with binoculars or small telescopes. The region contains various HII nebulae with the most prominent being RCW 119 (aka Sh 2-2, Gum 57) which forms a wind swept bubble caused by the eclipsing binary HD 153919. There are two other distinct nebula in the scene towards the right beyond the bubble. RCW 120 (aka Sh 2-3, Gum 58) appears as a 'S' shaped nebula with a dark nebula rift passing through it. Below this is the small, yet interesting planetary nebula known as the Bug Nebula due to its features (aka NGC 6302, Sh 2-6, Gum 60, RCW 124). The star cluster NGC 6281 resides 1,600 light years away, with most of the HII nebulosity much further in distance such as RCW 120 at 4,300 light years.
I will be honest, I had different intentions with this image. I acquired approximately 16hrs in total of Ha, OIII and SII data but found the area doesn't have a strong presence of OIII so didn't bother with a narrowband composite. I may consider working the data over just for fun, but there are other projects to move on to. The final result is noted as a HaRGB composite however I did blend a small amount of OIII into the areas where it was present in the raw master sub (done as a colour dodge blend mode). This gives the appearance of weak Ha+R blend alas it potentially a more accurate representation. I validated this with the base RGB master I use as a stars layer to confirm the areas were indeed less saturated in the red hue. I guess this all comes back down to a matter of taste but I'm fine with the result but the process need refinement. If you are wondering which star is HD 153919, its the bright one to very close to the lower left of the cluster NGC6281. The bubble/shock wave bow to the right is quite impressive. I'll try produce an annotated version when I get a chance. The Ha data set is certainly rich in detail. The bug nebula adds a cool dimension too. Not many other thoughts to add about this image. I defaulted back to MaximDL for pixel math Ha+R combine on the image as I had problems with CCDStack doing the task. Probable user error, I'll need to check it out again.
Thanks for checking it out. :)