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2024 年 4 月 15 日

哈伯与韦伯影像:雪茄星系
影像提供: NASA, ESA, CSA, STScI, Alberto Bolatto (UMD)

说明:这个星系发生了一些奇怪的事,但究竟是什么?编录号为M82的雪茄星系,其星系核会喷出泛红的发光气体和尘埃。尽管这个星爆星系,肯定不久前受到了邻居大螺旋星系M81接近的激发,但这并不能完全解释这些外泛红色发光气体和尘埃的来源。证据显示这些物质,是被众多恒星粒子风共同聚成的超级星系风所推送出去的。在这幅主题影像里,左侧图板呈现哈伯太空望远镜的可见光照片,右侧图板则是韦伯太空望远镜为此区中心所拍摄的红外光照片。仔细检视这幅韦伯新影像后,很意外的发现这些散发红光的尘埃与炽热的电浆有关。对这个奇特邻近星系本质的研究,势必会持续下去。



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2024 年 4 月 15 日

哈伯与韦伯影像:雪茄星系
影像提供: NASA, ESA, CSA, STScI, Alberto Bolatto (UMD)

说明:这个星系发生了一些奇怪的事,但究竟是什么?编录号为M82的雪茄星系,其星系核会喷出泛红的发光气体和尘埃。尽管这个星爆星系,肯定不久前受到了邻居大螺旋星系M81接近的激发,但这并不能完全解释这些外泛红色发光气体和尘埃的来源。证据显示这些物质,是被众多恒星粒子风共同聚成的超级星系风所推送出去的。在这幅主题影像里,左侧图板呈现哈伯太空望远镜的可见光照片,右侧图板则是韦伯太空望远镜为此区中心所拍摄的红外光照片。仔细检视这幅韦伯新影像后,很意外的发现这些散发红光的尘埃与炽热的电浆有关。对这个奇特邻近星系本质的研究,势必会持续下去。

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