Glowing Eye Nebula发光眼星云
![]() "Astronomers using NASA's Hubble Space Telescope have obtained images of the strikingly unusual planetary nebula, NGC 6751. Glowing in the constellation Aquila like a giant eye, the nebula is a cloud of gas ejected several thousand years ago from the hot star visible in its center. The Hubble observations were obtained in 1998 with the Wide Field and Planetary Camera 2 (WFPC2) by a team of astronomers led by Arsen Hajian of the U.S. Naval Observatory in Washington, DC. The Hubble Heritage team, working at the Space Telescope Science Institute in Baltimore, has prepared this color rendition by combining the Hajian team's WFPC2 images taken through three different color filters that isolate nebular gases of different temperatures. The nebula shows several remarkable and poorly understood features. Blue regions mark the hottest glowing gas, which forms a roughly circular ring around the central stellar remnant. Orange and red show the locations of cooler gas. The cool gas tends to lie in long streamers pointing away from the central star, and in a surrounding, tattered-looking ring at the outer edge of the nebula. The origin of these cooler clouds within the nebula is still uncertain, but the streamers are clear evidence that their shapes are affected by radiation and stellar winds from the hot star at the center. " (NASA description). Photo credit: NASA. 照片版权:NASA。
天文学家使用美国国家航空航天局(NASA)的哈勃太空望远镜,获得了行星状星云NGC 6751的图像。这个星云在天琴座中像一只巨大的眼睛般发光,是数千年 ago 从中心可见的热星发出的气体云。1998年,由美国海军天文台华盛顿分部的Arsen Hajian领导的天文学家团队,使用宽视场和行星相机2(WFPC2)在太空中获得了这些观测数据。哈勃遗产团队在巴尔的摩的太空望远镜科学研究所工作,通过三种不同颜色的滤光器,结合Hajian团队的WFPC2图像,制作了这张彩色图像,以突出星云中不同温度的气体。这个星云显示出一些令人印象深刻的、尚不完全理解的特征。蓝色区域标记的是温度最高的发光气体,形成围绕中心恒星残骸的大致圆形环。橙色和红色则显示了较冷气体的位置。较冷的气体倾向于沿着远离中心星的长丝状结构延伸,并在星云外围呈现出一片破碎的环状结构。这些较冷云团的起源仍不确定,但这些丝状结构清楚地表明它们的形状受到中心热星辐射和恒星风的影响。
发光眼星云 (NGC 6751) (NASA 图片) |
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