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林兹暗星云1251

(原标题: Lynds Dark Nebula 1251)

2025-07-10

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恒星正在林兹暗星云(LDN) 1251中形成。LDN 1251离我们大约1000光年远,漂浮在我们银河系的平面上方,它也被称为“腐鱼星云”。尘埃分子云是指向仙王座耀斑区域的暗星云复合体的一部分。在整个光谱中,对模糊的星际云的天文探索揭示了与新生恒星有关的能量冲击和流出,包括隐藏在图像中分散的赫比格-哈罗天体发出的红色光芒。遥远的背景星系也潜伏在场景中,几乎被埋在尘埃的背后。这个诱人的望远镜框架几乎跨越了天空中的三个满月。这相当于LDN 1251的估计距离超过25光年。

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Stars are forming in Lynds Dark Nebula (LDN) 1251. About 1,000 light-years away and drifting above the plane of our Milky Way galaxy, LDN 1251 is also less appetizingly known as "The Rotten Fish Nebula." The dusty molecular cloud is part of a complex of dark nebulae mapped toward the Cepheus flare region. Across the spectrum, astronomical explorations of the obscuring interstellar clouds reveal energetic shocks and outflows associated with newborn stars, including the telltale reddish glow from scattered Herbig-Haro objects hiding in the image. Distant background galaxies also lurk in the scene, almost buried behind the dusty expanse. This alluring telescopic frame spans almost three full moons on the sky. That corresponds to over 25 light-years at the estimated distance of LDN 1251.

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