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Tuesday, March 9, 2010

M1, the "Crab Nebula", finalized




Nebula in natural color. Narrowband channels are mixed to match visible spectrum. Red=80% H-alpha+20% S-II, Green=O-III and Blue=80% O-III+20% H-alpha to compensate otherwise missing H-beta.

Nebula in HST-palette, Red=S-II, Green=H-a and Blue=O-III

The Crab Nebula supernova remnant locates in constellation Taurus. The actual, bright, supernova was seen by Chinese and Arab astronomers in 1054.
Distance from Earth is about 6500 light years and diameter of the nebula is about 11 light years. Supernova remnant expands at a rate of about 1500 kilometers/second.
 
Last night I shot S-II channel and, for the first time, broadband luminance to show the broadband component in the nebula. There is a, 30 rounds per second spinning, massive, very magnetic,  neutron star in the core of the M 1. The hot plasma strikes existing gas, causing it glow in colors across the electromagnetic spectrum. Without broadband luminance, I can show only a part of the nebulas appearance.
 
Processing work flow:
Image acquisition, MaxiDL v5.07.
Stacked and calibrated in CCDStack.
Deconvolution with a CCDSharp, 30 iterations.
Levels, curves and color combine in PS CS3.
Broadband data is mixed to a narrowband channels in PS.

Telescope, Meade LX200 GPS 12" @ f5
Camera, QHY9 Guiding, SXV-AO @ 3Hz
Image Scale, 0,75 arcseconds/pixel
Exposures H-alpha 15x1200s, binned 1x1
O-III 2x1200s binned 2x2
S-II 3x1200s binned 1x1
Broadband luminance with a Hutec LP filter 2x1200s binned 1x1+ 3x600s binned 2x2

 

Sunday, March 7, 2010

M1, the "Crab nebula"


Nebula in natural color, composed from two narrowband channel, O-III & H-alpha.
This is a difficult target up here in North, due the smallish angular size and the low maximum elevation.
I shot final O-III frames when target was only about 20 degreen above horizont.
Seeing was better than few nights ago but not as good as I was hoping.
The Crab Nebula supernova remnant locates in constellation Taurus. The actual, bright, supernova was seen by Chinese and Arab astronomers in 1054.
Distance from Earth is about 6500 light years and diameter of the nebula is about 11 light years. Supernova remnant expands at a rate of about 1500 kilometers/second.
Processing work flow:
Image acquisition, MaxiDL v5.07.
Stacked and calibrated in CCDStack.
Deconvolution with a CCDSharp, 30 iterations.
Levels, curves and color combine in PS CS3.

Telescope, Meade LX200 GPS 12" @ f5
Camera, QHY9 Guiding, SXV-AO @ 3Hz
Image Scale, 0,75 arcseconds/pixel
Exposures H-alpha 15x1200s, binned 1x1
O-III 2x1200s binned 2x2
I'll shoot the S-II channel and more O-III later, when weather let me do so.

M1, the "Crab Nebula" as a Stereo Pair




Parallel vision


Cross vision

NOTE! This is a personal vision about forms and shapes, based on some known facts and artistic impression. Viewing instructions can be found from a Right hand side menu.
Original Image with details can be found HERE
Much more stereo images can be found HERE

M1, the "Crab Nebula" as an animated 3D-image

In this blog, there is lots of experimental material. To see my actual astroimages, please, see my Portfolio: http://astroanarchy.zenfolio.com/ Animations are made by creating artificial parallax to an image. Then two images are animated together by using conversion web service, Start3D. There can be some artifacts in images, due the experimental nature of this work! The volumetric models are based on some known facts and an artistic impression. Please, let the images load for few seconds to see them animated!
Original Image with details can be found HERE

M1, the "Crab Nebula" as a 3D-anaglyph (Red/Cyan)



An anaglyph Red/Cyan version.
You'll need Red/Cyan Eyeglasses to be able to see this image right. Note, if you have a Red and Green filters, you can use them! Red goes to Left eye.
NOTE! This is a personal vision about forms and shapes, based on some known facts and artistic impression

NGC 2175 & Sh2-252, the "Monkey head nebula" in HST-palette

Nebula in HST-palette, Red=S-II, Green=H-a and Blue=O-III

I managed to get the S-III channel information last night, just two 20min. frames.
That was enough to build the HST-palette image.

Technival details in previous post:
2 x 1200s S-II binned 2x2 added to a previous data.

Friday, March 5, 2010

NGC 2175 and Sh2-252, the "Monkey head nebula"




Nebula in natural color, composed from two narrowband channel, O-III & H-alpha.

There was some clear skys last night, so I was able to start a new project. this time my target is an open cluster, NGC 2175, it's surraunded by an emission nebula Sh2-252, it's sometimes called as a "Monkey head nebula".
NGC 2175 locates in constellation Orion. In my northern location, 65N, this target is not very high, about 40 degrees in maximum elevation. Distance from Oulu is about 6350 light years.
My original target was M1, the Crab Nebula but due the poor seeing i pick this secondary target. M1 needs a good seeing to be imaged well.

The nick name "Monkey head" is well deserved!

Processing work flow:
Image acquisition, MaxiDL v5.07.
Stacked and calibrated in CCDStack.
Deconvolution with a CCDSharp, 30 iterations.
Levels, curves and color combine in PS CS3.

Telescope, Meade LX200 GPS 12" @ f5
Camera, QHY9 Guiding, SXV-AO @ 3Hz
Image Scale, 0,75 arcseconds/pixel
Exposures H-alpha 7x1200s, binned 1x1
O-III 2x1200s binned 4x4
I'll shoot the S-II channel later, when ever weather let me do so, for this target.

Sh2-252, the "Monkey head nebula" as a Stereo pair

Parallel vision

Cross vision

NOTE! This is a personal vision about forms and shapes, based on some known facts and artistic impression. Viewing instructions can be found from a Right hand side menu.

Original Image with details can be found HERE
Much more stereo images can be found HERE

Sh2-252, the "Monkey face nebula" as an animated 3D-image

In this blog, there is lots of experimental material. To see my actual astroimages, please, see my Portfolio: http://astroanarchy.zenfolio.com/

Animations are made by creating artificial parallax to an image. Then two images are animated together by using conversion web service, Start3D.

There can be some artifacts in images, due the experimental nature of this work! The volumetric models are based on some known facts and an artistic impression.

Please, let the images load for few seconds to see them animated!


Original Image with details can be found HERE