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astronomyvocab
| Question | Answer |
|---|---|
| magelannic clouds | small irregular galaxies that are companions to the milky way |
| kiloparsec | a unit of distance equal to 1000pc, or 3,260ly |
| halo | the spherical region of a spiral galaxy that contains thing scattering of stars, clusters, and amounts of gas |
| nuclear bulge | the spherical cloud of stars that lies at the center of spiral galaxies |
| disk component | all material confined to the plane of the galaxy |
| spherical component | part of the galaxy including all matter in a spherical distributions around the center |
| spiral arms | long spiral patterns of light of bright stars, clusters, gas and dust extended from center to edge of disk |
| high velocity star | a star with large space velocity such stars are halo stars passing through at angles |
| rotation curve | a graph of orbital velocity versus radius in the disk of the galaxy |
| galactic corona | the low density extension of the halo of a galaxy |
| metals | all atoms heavier than helium |
| population I stars | stars rich in heavy metals than helium, relatively young, found in the disk of the galaxy |
| population II stars | poor in atoms heavier than helium, old, found in the halo or globular clusters |
| nucleosynthesis | the production of elements heavier than helium by fusion of atomic nuclei in stars |
| spiral tracers | objects used to map the spiral arms |
| density wave theory | proposed to account for spiral arms as compressions of the interstellar medium in the disk of the galaxy |
| flocculent | woolly, fluffy, used to refer to certain galaxies that have woolly appearances |
| self sustaining star formation | the process by which the birth of stars compresses the surrounding gas clouds and triggers the formation of more stars |
| sagittarius A | the powerful radio source located at the core of the milky way |
| keplarian motion | orbital motion in accord with Keplers laws of planetary motion |