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Monday, November 5, 2018

Sharpless 157 in Cassiopeia


I originally shot data for this Sharpless catalog object as Spring season 2018. I noticed that, I haven't publish a visual spectrum image out of it yet. So here we go, Sh2-157 in visual spectrum from narrowband channels.The mixture I'm using gives a very realistic color scheme. 

Red color is mixed by emission of an ionized hydrogen and Sulfur, 80% of H-alpha and 20% of S-II.
Green color is from the emission of an ionized oxygen, 100% of O-III
Blue color is mixed from the emission of an ionized oxygen and hydrogen, 85% of O-III and 15% of H-alpha. (The emission of an ionized hydrogen is added to compensate other wise missing H-beta emission.)

A mapped color version can be seen here:


A two frame mosaic of the Sharpless 157 (Sh2-157)
Please, click for a large image


Natural color scheme from the emission of an ionized elements, H-a, S-II and O-III
The photo width is about one degree of sky. (The full Moon covers about 0,5 degrees of the sky.)


An experimental starless version
Please, click for a large image


Details of the actual nebula stands out better in this experimental starless version.



close up
Please, click for a large image




INFO

Sharpless 157

The night sky between the constellations Cassiopeia and Cepheus is rich with nebulae and star clusters. The nebulae visible in this image include Sharpless 157 and Lynd’s Bright Nebula 537. The star clusters include Markarian 50 and NGC 7510. The planetary Nebula PLN 110-0.1 (WeSb) can be seen at lower left.

Sharpless 157 is sometimes referred to as the Lobster Claw Nebula for obvious reasons. The bright spot at upper left quarter of this photo is Lynd’s Bright Nebula (LBN) 537. Also designated at Sh 2 – 157a, it is a ring nebula around the Wolf-Rayet star WR 157.

At the lower right quarter of the image lays open star cluster NGC 7510.


With labels
Please, click for a large image




An older wide field photo of the area
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The area of a new photo is marked as a white rectangle. The Bubble nebula can be seen as a bluish pearl, just half a degree North West from the Sharpless 157. 
This photo is shot at 2007 with a QHY 8, a cooled astro camera and the Baader narrowband filter set, H-a, S-II and O-III. Tokina AT-X 300mm camera lens @ f2.8


Technical details

Processing work flow

Image acquisition, MaxiDL v5.07.
Stacked and calibrated in CCDStack2.
Deconvolution with a CCDStack2 Positive Constraint, 33 iterations, added at 50% weight
Color combine in PS CS3
Levels and curves in PS CS3.

Imaging optics
Celestron Edge HD 1100 @ f10 with 0,7 focal reducer for Edge HD 1100 telescope

Mount
10-micron 1000

Cameras and filters
Imaging camera Apogee Alta U16 and Apogee seven slot filter wheel
Guider camera, Lodestar x 2 and SXV-AOL

Astrodon filters,
5nm H-alpha 3nm S-II and 3nm O-III

Exposure times

H-alpha, 24 x 1200 s, binned 2x2 = 8 h
O-III, 10 x 1200 s, binned 4x4 = 3 h 20 min.
S-II, 9 x 1200 s. binned 4x4 = 3 h
Total 14 h 20 min

A single uncropped, calibrated and stretched 20 min. exposures as they come out from the camera.

H-alpha




S-II




O-III





LBN 239 and 243 in visual spectrum


Two of my latest photos are overlapping, so I was able to stitch them together to this two panel mosaic image.  This time in visual colors combined from narrowband channels, H-alpha, S-II and O-III. Mapped color version can be seen in my previous post HERE

LBN 239 and 243 in Constellation Cygnus
Please, click for a large image

Image is in Natural color palette from the emission of ionized elements, R=Hydrogen + Sulphur, G=Oxygen and B=Oxygen + 10% Hydrogen to compensate the missing H-beta emission.


Image info and the technical data

Exposure times, equipments, filters and processing information for the both frames in this two panel mosaic image can be found behind the links.

Upper part of the photo above:
https://astroanarchy.blogspot.com/2018/10/this-new-photos-shows-lbn-251-and.html

Bottom half:
https://astroanarchy.blogspot.com/2018/11/lbn-243.html


Sunday, November 4, 2018

LBN 239 and 243


Two of my latest photos are overlapping, so I was able to stitch them together to this two panel mosaic image. 


LBN 239 and 243 in Constellation Cygnus
Please, click for a large image

This two panel mosaic image is in mapped colours, from the emission of ionized elements, R=Sulphur, G=Hydrogen and B=Oxygen. 



Photos used for this mosaic image


Bow Tie of LBN 251, LBN 239 and the IC 1311
Click for a large photo


More info and technical detais, https://astroanarchy.blogspot.com/2018/10/this-new-photos-shows-lbn-251-and.html

LBN 243
Click for a large image



More info and technical detais, https://astroanarchy.blogspot.com/2018/11/lbn-243.html





Saturday, November 3, 2018

Just for a fun


Natural phenomenons has a tendency to have the same patterns.


Brain vessels VS Supernova remnant
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At left, a MRA-image of the human brain vessel system. At right, a supernova remnant Simeis 147 in constellation Taurus.

The MRA photo of brain vessels is form here:
https://www.nature.com/articles/d41586-018-07182-7

My photo of Simeis 147 supernova remnant can be seen here:
https://astroanarchy.blogspot.com/2013/09/a-supernova-remnant-simeis-147.html