What's in our galaxy?
Emission Nebulae Spectra consist of emission lines Are hot, ionised hydrogen plasma (plus a few other elements) where stars are born
Star Formation in Emission Nebulae
Dark Nebulae Cool molecular gas from which stars form Absorb (redden) the light from background stars Not a “hole” in space
Dark Nebulae in Emission Nebula
Reflection Nebulae – Found around hot O/B stars, scatter the light from the stars (no intrinsic emission)
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
Globular Clusters Old, and extremely dense spherical grouping of stars. Found orbiting outside our galaxy.
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
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
Veil nebula is 100,000 years old