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首页> 外文期刊>Space Science Reviews >Towards a Unified View of Inhomogeneous Stellar Winds in Isolated Supergiant Stars and Supergiant High Mass X-Ray Binaries
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Towards a Unified View of Inhomogeneous Stellar Winds in Isolated Supergiant Stars and Supergiant High Mass X-Ray Binaries

机译：朝着孤立的超巨星和超巨头高质量X射线二进制文件中的非均匀恒星风的统一视图

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Massive stars, at least similar to 10 times more massive than the Sun, have two key properties that make them the main drivers of evolution of star clusters, galaxies, and the Universe as a whole. On the one hand, the outer layers of massive stars are so hot that they produce most of the ionizing ultraviolet radiation of galaxies; in fact, the first massive stars helped to re-ionize the Universe after its Dark Ages. Another important property of massive stars are the strong stellar winds and outflows they produce. This mass loss, and finally the explosion of a massive star as a supernova or a gamma-ray burst, provide a significant input of mechanical and radiative energy into the interstellar space. These two properties together make massive stars one of the most important cosmic engines: they trigger the star formation and enrich the interstellar medium with heavy elements, that ultimately leads to formation of Earth-like rocky planets and the development of complex life. The study of massive star winds is thus a truly multidisciplinary field and has a wide impact on different areas of astronomy.
机译：巨大的恒星，至少类似于8倍的大于阳光，有两个关键的属性，使他们成为一个整体的星团，星系和宇宙的主要驱动因素。一方面，大量恒星的外层非常热，使它们产生大部分电离的星系的电离紫外线辐射;事实上，第一个大规模的恒星有助于在黑暗时期重新电离宇宙。巨大的恒星的另一个重要属性是他们生产的强大的恒星风和流出。这种质量损失，最后将大规模恒星作为超新星或γ射线爆发的爆炸，为壁炉间空间提供了大量的机械和辐射能量。这两种属性一起制作了大量的宇宙发动机之一：它们引发了明星的形成，并用重量的元素丰富了星际培养基，最终导致形成地球的岩石行星和复杂生活的发展。因此，大规模星风的研究是一个真正的多学科领域，对不同的天文区域产生了很大影响。

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