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What's in our galaxy?
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Emission Nebulae Spectra consist of emission lines
Are hot, ionised hydrogen plasma (plus a few other elements) where stars are born
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Star Formation in Emission Nebulae
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Dark Nebulae Cool molecular gas from which stars form
Absorb (redden) the light from background stars Not a “hole” in space
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Dark Nebulae in Emission Nebula
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Reflection Nebulae – Found around hot O/B stars, scatter the light from the stars (no intrinsic emission)
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Open Clusters Loose collection of stars
Gravitationally bound – all of the stars orbit each other – they are in the same region of space and were born in the same nebula
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Globular Clusters Old, and extremely dense spherical
grouping of stars. Found orbiting outside our galaxy.
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Planetary Nebulae Named for their disc-like appearance
They are the outer envelopes from the collapse of solar mass giant stars being ejected into space Normally spherical Contain a white dwarf star at their centre
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Supernova Remnants Ejecta from the explosion of a massive star
Crab nebula remnant is only 1000 years old At it's centre is a pulsar
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Veil nebula is 100,000 years old
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