词条 银河系核球
描述: 在银河系中,核球是银河系中心周围的区域,恒星在这里的排列具有一定体积,不像周围的盘状区域那么扁平。银河系的核球主要由年老恒星组成,但也混杂着年轻恒星。其他螺旋星系也有各不相同的中心核球结构。
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The OAE Multilingual Glossary is a project of the IAU Office of Astronomy for Education (OAE) in collaboration with the IAU Office of Astronomy Outreach (OAO). The terms and definitions were chosen, written and reviewed by a collective effort from the OAE, the OAE Centers and Nodes, the OAE National Astronomy Education Coordinators (NAECs) and other volunteers. You can find a full list of credits here. All glossary terms and their definitions are released under a Creative Commons CC BY-4.0 license and should be credited to "IAU OAE".
If you notice a factual or translation error in this glossary term or definition then please get in touch.
其他语言版本
- 阿拉伯语: الإنتفاخ المجرى
- 德语: Galaktischer Bulge
- 英语: Galactic Bulge
- 法语: Bulbe galactique
- 意大利语: Rigonfiamento galattico
- 日语: 銀河バルジ (外部链接)
- 韩语: 은하팽대부
- 马拉地语: तारकामंडळमधील
- 繁体中文: 銀河系核球



