Celestial hemisphere:  Northern  ·  Constellation: Taurus (Tau)  ·  Contains:  Crab nebula  ·  M 1  ·  NGC 1952  ·  Sh2-244
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The Crab Nebula, Gabe Shaughnessy
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The Crab Nebula

Getting plate-solving status, please wait...
The Crab Nebula, Gabe Shaughnessy
Powered byPixInsight

The Crab Nebula

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Description

The Crab Nebula is a supernova remnant that lies some 6500 light years away in the constellation Taurus. The nebula was discovered in 1731 and has the 1054 supernova event recorded by Chinese astronomers as its progenitor. At the heart of the nebula is the Crab Pulsar, which is a neutron star some 18 miles across and spins 30 revolutions per second. It emits very bright pulses of electromagnetic radiation from gamma rays on down to low energy radio waves. It's one of the brightest sources of high energy photons in the sky. The inner portion of the Crab Nebula has been shown to continue to expand, driven by the persistent pulsar wind.

For processing, I took a new route for me when combining the RGB and narrowband data. I used starnet to get RGB nebulosity, narrowband nebulosity, and RGB stars, then combined them with the pixel math expression

rgb_neb * rgb_wgt + nb_neb * (1 - rgb_neb * rgb_wgt) + rgb_stars

This expression accentuates narrowband data where there's little RGB data. This is the case for the OIII pillar structure on the top of the Crab, and fountain structure on the bottom. This also allows me to keep more of the RGB core of the Crab, which is more a pale white color. A simple addition of narrowband and rgb nebulosity would weaken the narrowband signal strength. In image C, I show the dependency on the rgb_wgt parameter, which varies from 0 (full nb + rgb stars) to 1. I also show the rgb image alone. I like rgb_wgt = 0.5, so went with that as my final version.

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