The Auriga Nebula

The Auriga Nebula
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The Auriga Nebula

The Aurigae Nebula, IC 405, also known as the Flaming Star Nebula, SH- 2-229 or caldwell 31 is an emission and reflection approximately 1,500 light-years from the solar system. This image was captured using the SPA-1-CMOS Takahashi FSQ-106ED and is pushing the limits of this telescopes field of view, with quite noticable star distortion at the corners. I dod not crop the image to show all of the beautiful Ha nebulosity.
SPECIFICATIONS
Telescope ..........................................................................................................................................................................................................................
Telescope
SPA-1 Takahashi FSQ-106ED
Camera ..........................................................................................................................................................................................................................
Camera
QHY 600
Location ..........................................................................................................................................................................................................................
Location
Oria Spain
Date of observation ..........................................................................................................................................................................................................................
Date of observation
28/03/23
Filters ..........................................................................................................................................................................................................................
Filters
Astrodon 3 nm Ha, Oiii, Sii all 10 x 600 sec
Processing ..........................................................................................................................................................................................................................
Processing
Pixinsight
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