AstroBin saves small pieces of text information (cookies) on your device in order to deliver better content and for statistical purposes. You can disable the usage of cookies by changing the settings of your browser. By browsing AstroBin without changing the browser settings, you grant us permission to store that information on your device.
I agreeImaging telescope or lens:Takahashi FSQ-106 ED
Imaging camera:Starlight Xpress SX-814 Trius Monochrome CCD
Mount:Sky-Watcher EZ-EQ6 GT
Guiding camera:Starlight-XPress Lodestar Autoguider
Software:Main Sequence Software Sequence Generator Pro, PIXINSIGHT 1.8, Photoshop CS6
Filters:Astrodon 3nm SII, Astrodon 3nm OIII, Ha 3nm, Blue, Green, Red
Accessories:Lakeside Astro Motor Focus System, Starlight Xpress SX 'Maxi wheel', Starlight Instruments FTF3545B-A Focuser
Resolution: 1664x1374
Dates:Dec. 17, 2017
Frames:
Astrodon 3nm OIII: 19x1800" bin 1x1
Astrodon 3nm SII: 4x1800" bin 1x1
Blue: 15x60" bin 1x1
Green: 15x60" bin 1x1
Ha 3nm: 20x1800" bin 1x1
Ha 3nm: 6x600" bin 1x1
Ha 3nm: 1x3600" bin 2x2
Red: 15x60" bin 1x1
Integration: 24.2 hours
Avg. Moon age: 28.83 days
Avg. Moon phase: 0.55%
Mean SQM: 18.50
Astrometry.net job: 1887947
RA center: 85.664 degrees
DEC center: 28.370 degrees
Pixel scale: 2.875 arcsec/pixel
Orientation: 0.258 degrees
Field radius: 0.862 degrees
Locations: The Hills Observatory, Manchester, United Kingdom
Data source: Backyard
Simeis 147, also known as the Spaghetti Nebula, SNR G180.0-01.7 or Sharpless 2-240, is a supernova remnant in the Milky Way, straddling the border between the constellations Auriga and Taurus.
The nebulous area is fairly large with an almost spherical shell and filamentary structure. The remnant has an apparent diameter of approximately 3 degrees, an estimated distance of approximately 3000 (±350) light-years, and an age of approximately 40,000 years.
It is believed that after its stellar explosion a rapidly spinning neutron star known as pulsar PSR J0538+2817 was left behind in the nebula core, emitting a strong radio signal.
Info from: https://en.wikipedia.org/wiki/Simeis_147
This image is a small section of the nebula, in fact it is panel 10 of a 16 panel mosaic that I started recently. Due to the rather long integration times for each panel, this mosaic will be considered a very long term project!
Narrow band images processed as tone maps with RGB stars added after. Most of the processing is done in PixInsight and finished off in Photoshop.
Comments