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WR 134的朦胧领域

(原标题: The Nebulous Realm of WR 134)

2026-05-22

浏览次数: 1536

这张宇宙快照覆盖了一个比满月宽两倍的视野,它位于飞翔的天鹅座的边界内。使用天文窄带滤光片拍摄的这张照片,突出了一个环状星云的明亮边缘,被电离的氢和氧气体所追踪。在这片广阔的星际云中,这些复杂的发光弧线是沃尔夫-拉叶星WR 134(图像中心附近最亮的恒星)的风吹来的物质外壳的部分。据距离估计,WR 134距离我们大约6000光年,使这个望远镜框架的直径超过100光年。在强大的恒星风中,大质量的沃尔夫-拉叶星以惊人的速度燃烧掉了它们的核燃料,以一颗壮观的超新星结束了它们大质量恒星演化的最后阶段。它们的恒星风和最后的超新星爆炸丰富了星际物质中的重元素,这些重元素将被纳入未来几代恒星中。

查看原文解释

This cosmic snapshot covers a field of view over twice as wide as the full Moon within the boundaries of the high-flying constellation Cygnus. Made using astronomical narrowband filters, the image highlights the bright edge of a ring-like nebula traced by the glow of ionized hydrogen and oxygen gas. Embedded in the region's expanse of interstellar clouds, the complex, glowing arcs are sections of shells of material swept up by the wind from Wolf-Rayet star WR 134, the brightest star near image center. Distance estimates put WR 134 about 6,000 light-years away, making this telescopic frame over 100 light-years across. Shedding their outer envelopes in powerful stellar winds, massive Wolf-Rayet stars have burned through their nuclear fuel at a prodigious rate and end their final phase of massive star evolution in a spectacular supernova. Their stellar winds and final supernova explosion enrich the interstellar material with heavy elements to be incorporated in future generations of stars.

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