A great thing about the ejection of matter from stars is that it seeds the galaxy with heavier elements formed by nuclear fusion in stars. If you look closely through a larger backyard telescope you may see the core of the original star that caused the nebula to form. At one time or another I've witnessed the magnitude 14.8 white dwarf stars at the center of the Ring Nebula in photographs I have taken at high exposure times. These white dwarfs are shining brightly to illuminate the surrounding gas.
Atoms and ions emit radiation when they are energized by incoming radiation. They emit only certain frequencies of radiation corresponding to different colours of the electromagnetic spectrum. A doubly ionized oxygen ion is found in abundance in planetary nebula and emits a certain spectra of light consisting of three emission lines around 500nm. This ion is also known as the (O III). Telescope stores stock O III filters that you can use on your eyepiece to allow the transmission of these lines. This allows an amazing amount of contrast of the nebula from the surrounding light pollution and stellar phenomena.
One of my favourite planetary nebulae is the Ring Nebula. It is located approximately halfway between Beta and Gamma Lyrae (the bottom of the Lyre). It is an extremely easy telescopic target to find and view. In dark skies you may even see it through a good set of binoculars. An image I took in Fall 2016 from my backyard is shown below.
M57 - Ring Nebula |
M57 in Lyra |
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