Veil Nebula - Gases Wave Storm, Charles Duarte FRAS

Veil Nebula - Gases Wave Storm

Veil Nebula - Gases Wave Storm, Charles Duarte FRAS

Veil Nebula - Gases Wave Storm

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Description

The rising intensity and recurrence of wave storm of gases can be observed from the supernova remnant is known as the  Veil Nebula also called the Cirrus Nebula or the Filamentary Nebula.The nebula’s progenitor star is not visible  — which was 20 times the mass of the Sun — lived fast and died young, ending its life in a cataclysmic release of energy.Despite this stellar violence, the shockwaves and debris from the supernova sculpted the nebula’s delicate tracery of ionized gas — creating a scene of surprising astronomical beauty yet we observatory the similarity to an sea ocean wave storm.To create this colorful image, of the Veil Nebula observations is taken from my observatory in Southern Spain, using a OS 1400mm x 250mm telescope, the camera is a FLI16803, three different filters (Ha, OIII, SII) were used.

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Veil Nebula - Gases Wave Storm, Charles Duarte FRAS