(astronomy) A morphological feature of some spiral galaxies that appears similar to a conventional galaxy bulge, but with internal dynamics that are dominated by rotation rather than random motions..
현재 검증된 한국어 뜻은 준비 중이며 영어 정의는 “(astronomy) A morphological feature of some spiral galaxies that appears similar to a conventional galaxy bulge, but with internal dynamics that are dominated by rotation rather than random motions.”입니다.