Wolf-Rayet 星 124

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• 原始文章：Wolf-Rayet 124
• 影像來源：NASA, ESA, CSA, STScI, Webb ERO Production Team
• 台文翻譯：An-Li Tsai (NCU)

[漢羅] Wolf-Rayet 星 124

這張 清楚 ê 紅外線景色 是高溫明亮 ê Wolf-Rayet 星 124 強烈 ê 恆星風 驅動、推捒四箍圍仔 ê 氣體 kah 塗粉。 這个引人注目 ê 六指光尖 ê 圖樣，其實是對應到恆星 ê 影像。 會生做這形是因為 James Webb 太空望遠鏡 是 ùi 18 塊六角形鏡組成--ê。 WR 124 離咱差不多 1 萬 5000 光年遠，就 tī 北方 ê 天箭座遐。 伊 ê 質量是有超過 30 倍 ê 太陽質量。 這个恆星 ê 掣流 星雲差不多有 6 光年闊，是 tī 咱銀河系內底揣會著 ê 一款 tī 懸質量恆星演化 過程一个較短嘛較罕得看--著 ê 階段。 這暗示講，WR 124 隨會以超新星爆炸 ê 方式，結束恆星 ê 性命。 超新星爆炸留--落來 ê 厚塗粉星際殘骸，是 tī 脹大 ê 星雲內底 形成--ê。 這 會影響著 後一个世代 ê 恆星形成。

[POJ] Wolf-Rayet chheⁿ 124

Chit tiuⁿ chheng-chhó ê âng-gōa-sòaⁿ kéng-sek sī ko-un bêng-liōng ê Wolf-Rayet chheⁿ 124 kiông-lia̍t ê hêng-chheⁿ-hong khu-tōng, thui-sak sì-kho͘-ûi-á ê khì-thé kah thô͘-hún. Chit ê ín-lâng-chù-bo̍k ê la̍k-cháiⁿ kng-chiam tô͘-iūⁿ, kî-si̍t sī tùi-èng kàu hêng-chheⁿ ê iáⁿ-siōng. Ē seⁿ-chò chit hêng sī in-ūi James Webb thài-khong bōng-oán-kiàⁿ sī ùi 18 tè la̍k-kak-hêng kiàⁿ cho͘-sêng--ê. WR 124 lī lán chha-put-to 1 bān 5000 kng-nî hn̄g, to̍h tī pak-hong ê Thian-chìⁿ-chō hiah. I ê chit-liōng sī ū chhiau-kòe 30 pōe ê thài-iông chit-liōng. Chit ê hêng-chheⁿ ê chhoah-lâu seng-hûn chha-put-to ū 6 kng-nî khoah, sī tī lán Gîn-hô-hē lāi-té chhōe-ē-tio̍h ê chi̍t-khoán tī koân-chit-liōng hêng-chheⁿ ián-hòa kòe-têng chi̍t-ê khah té mā khah hán-tit khòaⁿ--tio̍h ê kai-tōaⁿ. Che àm-sī kóng, WR 124 sûi ē í chhiau-sin-seng po̍k-chà ê hong-sek, kiat-sok hêng-chheⁿ ê sèⁿ-miā. Chhiau-sin-seng po̍k-chà lâu--lo̍h-lâi ê kāu thô͘-hún seng-chè chân-hâi, sī tī tiùⁿ-tōa ê 星雲 lāi-té hêng-sêng--ê. Che ē éng-hióng tio̍h āu chi̍t ê sè-tāi ê hêng-chheⁿ hêng-sêng.

[KIP] Wolf-Rayet tshenn 124

Tsit tiunn tshing-tshó ê âng-guā-suànn kíng-sik sī ko-un bîng-liōng ê Wolf-Rayet tshenn 124 kiông-lia̍t ê hîng-tshenn-hong khu-tōng, thui-sak sì-khoo-uî-á ê khì-thé kah thôo-hún. Tsit ê ín-lâng-tsù-bo̍k ê la̍k-tsáinn kng-tsiam tôo-iūnn, kî-si̍t sī tuì-ìng kàu hîng-tshenn ê iánn-siōng. Ē senn-tsò tsit hîng sī in-uī James Webb thài-khong bōng-uán-kiànn sī uì 18 tè la̍k-kak-hîng kiànn tsoo-sîng--ê. WR 124 lī lán tsha-put-to 1 bān 5000 kng-nî hn̄g, to̍h tī pak-hong ê Thian-tsìnn-tsō hiah. I ê tsit-liōng sī ū tshiau-kuè 30 puē ê thài-iông tsit-liōng. Tsit ê hîng-tshenn ê tshuah-lâu sing-hûn tsha-put-to ū 6 kng-nî khuah, sī tī lán Gîn-hô-hē lāi-té tshuē-ē-tio̍h ê tsi̍t-khuán tī kuân-tsit-liōng hîng-tshenn ián-huà kuè-tîng tsi̍t-ê khah té mā khah hán-tit khuànn--tio̍h ê kai-tuānn. Tse àm-sī kóng, WR 124 suî ē í tshiau-sin-sing po̍k-tsà ê hong-sik, kiat-sok hîng-tshenn ê sènn-miā. Tshiau-sin-sing po̍k-tsà lâu--lo̍h-lâi ê kāu thôo-hún sing-tsè tsân-hâi, sī tī tiùnn-tuā ê 星雲 lāi-té hîng-sîng--ê. Tse ē íng-hióng tio̍h āu tsi̍t ê sè-tāi ê hîng-tshenn hîng-sîng.

[English] Wolf-Rayet 124

Driven by powerful stellar winds, expanding shrouds of gas and dust frame hot, luminous star Wolf-Rayet 124 in this sharp infrared view. The eye-catching 6-spike star pattern is characteristic of stellar images made with the 18 hexagonal mirrors of the James Webb Space Telescope. About 15,000 light-years distant toward the pointed northern constellation Sagitta, WR 124 has over 30 times the mass of the Sun. Produced in a brief and rarely spotted phase of massive star evolution in the Milky Way, this star's turbulent nebula is nearly 6 light-years across. It heralds WR 124's impending stellar death in a supernova explosion. Formed in the expanding nebula, dusty interstellar debris that survives the supernova will influence the formation of future generations of stars.

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