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Saturday, December 15, 2012

Soul Nebula, up close & personal



In this blog post of mine, I'm showing a collection of the Soul Nebula images. Some of them are shot in previous years and some at this Autumn season. All images are reprocessed since I have now a better technique.

IC 1848, the "Soul Nebula"
Ra 02h 51m 36.24s Dec +60° 26′ 53.9"



Image is in mapped colors, from the emission of ionized elements,
 R=Sulfur, G=Hydrogen and B=Oxygen.



Soul nebula in wider field image

In this wide field image, the Soul Nebula is shown with its neighbor, the Heart nebula.
Image is shot with the Canon EF 200mm f1.8 lens, Baader narrowband filters and the QHY9 cooled astronomical camera. 


Info

Soul Nebula, (Sh2-199, LBN 667) is an emission nebula in constellation Cassiopeia. IC 1848 is a cluster inside Soul Nebula. Distance is about 7.500 light years. This complex is a Eastern neighbor of IC 1805, the "Heart Nebula" and they are often mentioned together as Heart and Soul.


Closeups of the Soul Nebula
Images are shot with a Meade LX200 12" telescope

Image is in mapped colors, from the emission of ionized elements,
 R=Sulfur, G=Hydrogen and B=Oxygen.






Image is in mapped colors, from the emission of ionized elements,
 R=Sulfur, G=Hydrogen and B=Oxygen.





A two frame mosaic from previous images.



Image is in mapped colors, from the emission of ionized elements,
 R=Sulfur, G=Hydrogen and B=Oxygen.






Orientation

The previous closeups are marked in this image as a white rectangles.



A collection of images in visual spectrum
Natural color composition from the emission of ionized elements, R=80%Hydrogen+20%Sulfur, G=100%Oxygen and B=85%Oxygen+15%Hydrogen to compensate otherwise missing H-beta emission. This composition is very close to a visual spectrum.










Technical details

All technical data for the mages in this blog post can be found from my portfolio.







Thursday, December 13, 2012

The Pelican Nebula reprocessed




I reprocessed this image since weather doesn't support imaging up here and my processing work flow is somehow different now. My new work flow produces much softer images, I think.


The "Pelican Nebula"
Ra 20h 50m 48s Dec +44° 20′ 60"

Sh2-142 alias NGC 7380, in mapped colors, from the emission of ionized elements,
 R=Sulfur, G=Hydrogen and B=Oxygen.




A closeup



Info

The Pelican Nebula (also known as IC5070 and IC5067) is an Hydrogen emission region associated with the North America Nebula in the constellation Cygnus. The nebula resembles a pelican in shape, hence the name. The Pelican Nebula is , close to Deneb, and divided from its brighter, larger neighbor, the North America Nebula, by a molecular cloud filled with dark dust. Distance is about 1800 light years


Natural color composition from the emission of ionized elements, R=80%Hydrogen+20%Sulfur, G=100%Oxygen and B=85%Oxygen+15%Hydrogen to compensate otherwise missing H-beta emission. This composition is very close to a visual spectrum.


Orientation

The area of interest is marked with a white rectangle. This image shows a large portion of constellation Cygnus, North America Nebula, NGC 7000 at right and Pelican Nebula at left. This image is a small part of very large mosaic image of the Cygnus. 


Image showing a light emitted by the ionized Hydrogen, H-alpha

A H-alpha channel alone


Technical details

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.

Camera QHY9, 
Optics Meade LX200 GPS 12" forced to @ f4.65 
Guiding with SXV-AO active optics unit 11Hz 
Filters 
Baader H-alpha 7nm, 6h, 20 min subs 
Baader O-III 8,5nm 1h, 10 min. subs binned 3x3 
S-II 1,40h, 10 min subs binned 3x3

Original processing can be seen here:



Ps.

A study about an apparent size in the sky

More info in here: 

The size of the Moon (0.5 degrees) is marked at first image in the series.




Wednesday, December 12, 2012

The Wizard Nebula reprocessed



I reprocessed this image since weather doesn't support imaging up here and my processing work flow is somehow different now. My new work flow produces much softer images, I think.



NGC 7380, Sh2-1142, the "Wizard Nebula", in Cepheus
Ra 22h 47m 0s Dec +58° 06′ 00″

Sh2-142 alias NGC 7380, in mapped colors, from the emission of ionized elements,
 R=Sulfur, G=Hydrogen and B=Oxygen.





A closeup




Info


NGC 7380 is a catalog number of  the open star cluster inside Wizard nebula, SH2-142.
Nebula locates in constellation Cepheus, about 7000 light years from my home. 



Natural color composition from the emission of ionized elements, R=80%Hydrogen+20%Sulfur, G=100%Oxygen and B=85%Oxygen+15%Hydrogen to compensate otherwise missing H-beta emission. This composition is very close to a visual spectrum.



An experimental starless version

This image shows just the gas formation, without stars interfering. 



Previous version
same raw data is used here





Technical details:

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 @ 6,5Hz
Image Scale, 0,75 arcseconds/pixel
Exposures H-alpha 15x1200s, binned 1x1
S-II 1x1200s, binned 4x4
O-III 1x1200s, binned 4x4
Beside data here, a color information from an older wide field image is used.
Image can be seen here: http://astroanarchy.blogspot.fi/2011/02/sh2-142-wizard-nebula-wide-field.html



A study about an apparent scale in a sky







Monday, December 10, 2012

Elephant's Trunk nebula reprocessed



Weather doesn't support any imaging, so I reprocessed an older image, the Elephant's Trunk nebula.


Elephant's Trunk
A detail in IC 1396 emission nebula

Image in mapped colors from the light emitted by ionized elements. 
Red=Sulfur, Green=Hydrogen and Blue=Oxygen.
Buy a photographic print from HERE

The elephant's Trunk nebula is a concentration of interstellar gas and dust in the star cluster IC 1396.
This ionized gas region locates in the constellation Cepheus about 2400 light years away.
Formation is coursed by a stellar wind, radiation pressure, from a group of massive young stars.



Natural color composition from the emission of ionized elements, R=80%Hydrogen+20%Sulfur, G=100%Oxygen and B=85%Oxygen+15%Hydrogen to compensate otherwise missing H-beta emission. This composition is very close to a visual spectrum.
Buy a photographic print from HERE

A detail

At the time of imaging, the seeing was very good, HWFM ~2.5


A wide field image of the area
The Trunk formation at bottom middle

More info about this image HERE.
Buy a photographic print from HERE


A Gargoyle of the sky

A Gargoyle?..    See HERE




Technical details

All technical details are with an original image HERE