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Supernova Remnants, Gary Imm

Supernova Remnants

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Supernova Remnants, Gary Imm

Supernova Remnants

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Description

Supernova remnants (SNR) are some of the most fantastic objects in the sky.  The fine tendrils seen throughout each nebula are ionized gas fronts, ejected as shock waves in the supernova explosion. The different colors reflect the variations in the strengths and compositions of these gas shock waves. Each SNR continues to expand outward, changing the details of its appearance slightly each year. These SNRs are typically thousands of years old.  

The use of narrowband filters is required in order to bring out the color and detail of these nebulae.  The filters typically used to capture the SNR signal are hydrogen, oxygen and sulfur.  Most of these images use the bi-color HOO palette. 

Over 300 SNRs have been catalogued in our Milky Way.  The poster contains the SNRs that I have been able to image to date.   The technical data for the objects on the poster is shown in Revision E.

Each of the objects of the poster has previously been uploaded and described individually on Astrobin. They all reside in my Astrobin SNR Collection.

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Revisions

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Description: Technical Data

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Description: Object Locations

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Supernova Remnants, Gary Imm