Glossary term: 星雲
Description: 星雲是一種遙遠的天體,具有雲的外觀。通常,星雲由星際氣體和塵埃組成。在歷史上,星雲一詞指的是所有延展的、邊緣模糊的天體,包括我們今天所認識的星系--像銀河系這樣的遙遠恆星系統。如今,星雲一詞僅限於指代星際介質中的氣體和塵埃雲,即星系內恆星之間的氣體和塵埃。星雲被分為許多不同的種類:分子雲相對較冷,顏色較暗,主要由分子氫組成;新的恆星就是在這樣的雲中形成的。巨型分子雲可以包含多達數百萬個太陽質量的氫氣。年輕恆星頻繁地噴射出狹窄的電離氣體噴流;當這些噴流激發周圍的氣體時,就會形成一種叫做赫比-哈羅(Herbig–Haro)天體的星雲。當大質量恆星形成後,它們的強烈輻射會使周圍的氣體髮出特徵性的紅光;這種由熾熱的電離氫氣組成的星雲被稱為 HII 區(電離氫區)。其他類型的星雲與恆星的死亡有關:低質量恆星的死亡會留下不斷膨脹的氣體外殼,這種星雲(命名上有些令人困惑)被稱為行星狀星雲。當大質量恆星以超新星的形式爆發時,噴出的氣體會形成一種叫做超新星遺跡的星雲。
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Term and definition status: The original definition of this term in English have been approved by a research astronomer and a teacher The translation of this term and its definition is still awaiting approval
This is an automated transliteration of the simplified Chinese translation of this term
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