jase
24-07-2007, 03:07 PM
Hi All,
I am pleased to present the galactic plane wanderers NGC6357 and NGC6334 (http://www.cosmicphotos.com/gallery/image.php?fld_image_id=108&fld_album_id=11).
Within the constellation Scorpios, two magnificent nebulae wander along the galactic plane of the Milky Way galaxy. Four 7th magnitude stars perfectly aligned point to the center of the faint emission nebula NGC6357 (left in frame). The nebula forms the shape of a crab and is approximately 5500 light-years distant. A feline footprint marks NGC6334 (right in frame). It’s commonly known as the Cat’s Paw nebula.
Both NGC6357 and NGC6334 nebulae are close the the galactic plane and as such are hidden by galactic dust which makes them difficult to observe visually. The galactic dust decreases the blue and green wavelength emissions (colour extinction). This is evident by the stars within the nebulosity – there are no obvious signs of bright blue stars commonly found in star forming regions. The galactic dust particles are selectively removing blue light – a phenomenon known as “interstellar reddening”. The dust particles have very little effect on red light wavelengths hence the nebulae glows vibrantly in the hydrogen alpha emission line.
Info on the image and processing;
Total exposure time: 4.2 hours (Luminance:105min, R:50min, G:50min, B:50min). The image is an LLRGB composite. This object is best suited for Ha imaging, but looks still impressive with strong luminance data. May revisit to get Ha data another time. Thanks glenc for the nebula listing - these two objects pair beautifully in the frame of the FSQ/STL11k combo.
Subtly different routine from that what I normally do for LLRGB images. Typically, I use the PS shadow/highlights tool to perform the non-linear stretch on the RGB data, but this time I used DDP as I felt it was more suited to the strong luminance info. I still manually stretched the luminance data with PS levels and curves. The luminance data was placed through two iterations of LR deconvolution. A few PS layer masks created in the routine – a star only layer, two nebula layers to manage colours and finally a high pass. Noise reduction also performed through an inverted layer mask.
OT: Please note that I’m updating my gallery web code and as such image links to my previous posts will become invalid. I will update what I can in due time. The new code improves image scaling and management amongst other things. I’m not happy with the PHP GD library that handles the dynamic resizing of images as it introduces a lot of compression artifacts. If I can’t get the results I want, I will revert back to my original code. I will continue to work on it when I get the time. Minor disruptions may occur during the upgrade period - sorry for any inconvenience.
Thanks for looking. I hope you enjoy it. All comments welcome.:)
I am pleased to present the galactic plane wanderers NGC6357 and NGC6334 (http://www.cosmicphotos.com/gallery/image.php?fld_image_id=108&fld_album_id=11).
Within the constellation Scorpios, two magnificent nebulae wander along the galactic plane of the Milky Way galaxy. Four 7th magnitude stars perfectly aligned point to the center of the faint emission nebula NGC6357 (left in frame). The nebula forms the shape of a crab and is approximately 5500 light-years distant. A feline footprint marks NGC6334 (right in frame). It’s commonly known as the Cat’s Paw nebula.
Both NGC6357 and NGC6334 nebulae are close the the galactic plane and as such are hidden by galactic dust which makes them difficult to observe visually. The galactic dust decreases the blue and green wavelength emissions (colour extinction). This is evident by the stars within the nebulosity – there are no obvious signs of bright blue stars commonly found in star forming regions. The galactic dust particles are selectively removing blue light – a phenomenon known as “interstellar reddening”. The dust particles have very little effect on red light wavelengths hence the nebulae glows vibrantly in the hydrogen alpha emission line.
Info on the image and processing;
Total exposure time: 4.2 hours (Luminance:105min, R:50min, G:50min, B:50min). The image is an LLRGB composite. This object is best suited for Ha imaging, but looks still impressive with strong luminance data. May revisit to get Ha data another time. Thanks glenc for the nebula listing - these two objects pair beautifully in the frame of the FSQ/STL11k combo.
Subtly different routine from that what I normally do for LLRGB images. Typically, I use the PS shadow/highlights tool to perform the non-linear stretch on the RGB data, but this time I used DDP as I felt it was more suited to the strong luminance info. I still manually stretched the luminance data with PS levels and curves. The luminance data was placed through two iterations of LR deconvolution. A few PS layer masks created in the routine – a star only layer, two nebula layers to manage colours and finally a high pass. Noise reduction also performed through an inverted layer mask.
OT: Please note that I’m updating my gallery web code and as such image links to my previous posts will become invalid. I will update what I can in due time. The new code improves image scaling and management amongst other things. I’m not happy with the PHP GD library that handles the dynamic resizing of images as it introduces a lot of compression artifacts. If I can’t get the results I want, I will revert back to my original code. I will continue to work on it when I get the time. Minor disruptions may occur during the upgrade period - sorry for any inconvenience.
Thanks for looking. I hope you enjoy it. All comments welcome.:)