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"The nebula appears to have distinct regions that capture different phases of its evolution — an outer shell of gas that was blown off first and consists mostly of hydrogen, and an inner cloud with more structure that contains a mix of different gases," NASA's blog post reads. The dark line that runs vertically through the nebula, giving it the cranial appearance, could be the result of "an outburst or outflow from the central star, which typically occurs as twin jets burst out in opposite directions." Both Webb's Near-Infrared Camera (NIRCam) and its Mid-Infrared Instrument (MIRI) were used to document the nebula.。业内人士推荐heLLoword翻译官方下载作为进阶阅读
pubmed.ncbi.nlm.nih.gov。关于这个话题，safew官方版本下载提供了深入分析
📚 十大经典排序算法 C语言笔记（一看就会版）
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