Celestial hemisphere:  Southern  ·  Constellation: Vela (Vel)  ·  Contains:  e Vel
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Filaments of Vela, Bogdan Borz
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Filaments of Vela

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Filaments of Vela, Bogdan Borz
Powered byPixInsight

Filaments of Vela

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Description

The Vela supernova remnant is a supernova remnant in the southern constellation Vela. Its source Type II supernova exploded approximately 11,000–12,300 years ago (and was about 800 ly away). The association of the Vela supernova remnant with the  Vela pulsar, made by astronomers at the University of Sydney in 1968, was direct observational evidence that supernovae form neutron stars.The Vela supernova remnant includes NGC 2736. It also overlaps the Puppis A supernova remnant, which is four times more distant. Both the Puppis and Vela remnants are among the largest and brightest features in the X-ray sky.The Vela supernova remnant (SNR) is one of the closest known to us. (Source: Wikipedia)

I processed the data provided by Martin Pugh on his site, taken at the Observatory in New South Wales, Australia. It is not an easy target to process in SHO (this is a narrowband composition with RGB stars), the classic SHO palette generates pretty weird and unusual colors. So I did a lot of experimenting in Pixelmath, finally sticking to a specific dynamic factor based on SII and Ha for the R channel and a dynamic factor based on Ha and OIII for the G channel. The structures in Vela remind me of the architecture of the Universe modelled on the observation of clusters of galaxies in Laniakea and beyond.

Data acquistion and calibration: Martin Pugh
Post-treatment: Bogdan Borz 

Ha 19 x 1800s
SII 21 x 1800s
OIII 11 x 1800s
R 4 x 600s
G 3 x 600s
B 3x600s
Total exposure : 27h 40m

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