Abstract
A planetary nebula is formed at the end of the life of a star which has a mass about equal to that of our Sun. Any much more massive star cannot pass through this relatively gentle stage; it explodes in a shattering supernova. A star much less massive than the Sun simply fades out slowly, like an ember from a campfire. As you look out into the Milky Way, over half of the stars you see will pass through this planetary nebula phase as their final curtain call.
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© 2000 Springer-Verlag London
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Coe, S.R. (2000). What Can Be Seen Within Planetary Nebulae ?. In: Deep Sky Observing. Patrick Moore’s Practical Astronomy Series. Springer, London. https://doi.org/10.1007/978-1-4471-0365-3_12
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DOI: https://doi.org/10.1007/978-1-4471-0365-3_12
Publisher Name: Springer, London
Print ISBN: 978-1-85233-627-1
Online ISBN: 978-1-4471-0365-3
eBook Packages: Springer Book Archive