Labels:daily | reckoner | sky OCR: ble, their the spiral arms are vis structure is difficult to form Clumpy and filamenta itire disk ations range over the of the galaxy star Clearly, there is side than fornation on the right a.xy This in other parts of the ined partly region is so sharply de in between because of an interacti galactic the galaxy and the inte case medium which in thi gas insideunusually dense Whe the inter- the galaxy collides witl sulting galactic med um, the stinct shocl wave crea tes also galactic border and ma trigger star forrna ation spira forn unpy ntire righ sharpl beca LUSE ilactic galax liun usuall lactic actic
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