Here’s my rendition of the famous Pelican Nebula, the Ha rich neighbor of NGC7000. It took four hours in 15-minute subframes to accomplish this decently clean and signal rich image.
2000 light-years away, it’s a very active star forming region.
Here’s my rendition of the famous Pelican Nebula, the Ha rich neighbor of NGC7000. It took four hours in 15-minute subframes to accomplish this decently clean and signal rich image.
2000 light-years away, it’s a very active star forming region.
Only three hours could go into the making of this peculiar portrait, picturing the beautiful Bubble Nebula, aka NGC7635, and the bright open cluster M52.
The Bubble is an area of ionized hydrogen, currently being blown away by the stellar wind of a massive and hot central star, whose mass is believed to be twenty to forty times that of our Sun. The Bubble extends over a diameter of about 10 light-years, lies 11000 light-years away and is a set for very violent and turbulent processes at work.
Four hours and forty-five minutes went into the making of this rendering of the Elephant’s Trunk, part of the nebulosity around the open cluster IC1396.
The elongated cloud you see in the image, resembling the trunk of an elephant, is really over 20 light-years long, and the whole complex is 2400 light-years away from Earth.
This bright emission area is thought to be a star forming region.
Here’s a humble attempt to reprocessing the Crescent I did with Gustaaf Prins and (waiting for clearance to disclose name). It’s a composition of red, green, blue, Ha, SII and OIII channels.
Of course when performing this kind of processing, there is usually no pretense of achieving real natural colors. The problems lies mostly in two factors: first, the Ha and SII channels are both reddish, while the OIII channel is greenish blue; second, the intensity of the signal at different bandwidths varies considerably, and if you don’t want to end up with a very color-unbalanced imaged, you need to stretch different channels differently.
This image uses red, Ha and SII (mixed in different percentages) for the red channel, green and OIII for the green channel, and blue, OIII and a pinch of Ha for the blue channel.
Here are seven an a half hours, split in fifteen 30-minute subs, on the Wizard Nebula, aka NGC7380, aka Sh2-142.
NGC 7380 is a typical starforming region in the direction of an outer spiral arm of our galaxy (around 7,000 light years distant). This field contains many young energetic stars that make the natal gas that surround them glow an intense pink/red. The majority of stars for this newly formed group are out of the field to the upper left (right, in my image). Their winds and radiation sculpt clouds of gas and dust into the mountainous ridges seen here. The darkest parts of this image are foreground clouds of dust thick enough to extinct the light beyond them
(Quoted from http://www.noao.edu/outreach/aop/observers/n7380.html)
Only 100 minutes went into the capturing of this NGC7000, split into five 20-minute subs. Obviously this is an area extremely rich of hydrogen, as the amount of signal is incredible for my tiny 80mm refractor.
NGC7000, aka The North America nebula (obvious nickname), is a very large nebula, actually covering an area four times as large as the full moon. The area I imaged is called “Cygnus’s Wall”.
Very interesting, the shape you see is not the result of a particularly shaped cloud of gas, but it’s determined by the fact that between us and NGC7000 lie some bands of interstellar dark dust.
The distance of the nebula is not known, nor is the star that lights it. Some sources indicate that the star might be Daneb; in that case, NGC7000 might be 1800 light-years away, and it’s absolute size would be about 100 light-year across.
Thanks to my friend Milosz, my M27 has been gifted with some twelve and a half hours of pretty good old h-alpha signal. I have here merged that data to my Red channel, and composed the image above with PixInsight.