Warwick Astronomy & Astrophysics Consolidated Grant 2023-2026

恒星、行星和星系是如何形成的？它们是如何进化的，它们是如何死亡的？华威大学的天文学和天体物理学小组通过对大小型望远镜的观测，以及物理驱动的计算模型来研究这样的问题。光学望远镜在天文学中的使用可以追溯到伽利略400多年前，但我们现在正处于一个新的伽利略发现时代，直到2015年才首次探测到引力波(GWS)。GW提供了一种完全不同的宇宙观，深入研究了最极端事件的核心，这些事件被称为密度超乎想象的恒星螺旋聚集在一起，在合并前的最后一刻，它们的能量输出与整个可观测宇宙的其余部分相媲美。GW望远镜可以一次看到几乎所有的地方，但具有相当于非常模糊的视野。为了精确定位来源，我们需要用电磁(EM)，即光学、射电和X射线望远镜来观察它们，但即使是这样也很困难，因为你必须知道首先去哪里寻找。在华威，我们正在研究一种名为后藤的望远镜来做这件事。从欧洲和澳大利亚的网站来看，Goto的设计具有宽广的视野和速度，可以在探测到宇宙中最快、最猛烈的事件后几分钟内追踪它们。在我们所在的银河系内，许多威力较小但寿命较长的天体发出离地球更近的GW。我们正在开始从电磁观测中寻找系统，这些系统也将作为来自太空的GW源被探测到。这些都是奇异的来源：其中一个由两颗恒星组成，每颗恒星的大小都是地球的大小，但质量是地球的10万倍，这两颗恒星相互环绕的时间只有五分钟多一点。我们将使用安装在大型光学望远镜上的专业高速相机来研究它们，以探索它们是如何进化的，以及了解它们的数量和它们是如何形成的重要一步。引力波给了我们对宇宙的新视角，但新的仪器和技术几乎做了同样的事情。1995年，通过一种叫做光谱学的古老天文学工具的特别敏感的应用，第一颗系外行星被发现。从那时起，在各种令人眼花缭乱的星系中发现了数以千计的行星，其中许多与我们的太阳系非常不同。在华威，我们长期以来一直在利用地球和太空中的两台望远镜发现系外行星，并将在这次拨款中这样做，以了解当行星靠近其宿主恒星时，可能会摧毁或侵蚀行星的过程。许多已知的系外行星距离它们的主恒星很近，但这在一定程度上是因为我们如何找到它们，所以我们的另一项研究旨在将行星探测推向更广泛的轨道，更接近我们太阳系的轨道。沃里克对欧空局领导的一项名为柏拉图的新太空任务非常感兴趣，该任务将为这项工作提供戏剧性的推动。柏拉图有很大的视野，可以捕捉到围绕最亮恒星运行的行星。这些都是关键目标，因为它们就在附近，但最重要的是，它们允许更具挑战性的光谱应用，足以让我们探测行星大气的真正组成。地球和太阳系的其他行星是由年轻太阳周围的物质盘形成的，这些物质以行星本身的形式存在，但也以彗星、小行星和尘埃的形式存在。我们的目标是寻找其他恒星周围类似结构的证据，特别是从它们散射星光的尘埃中寻找证据。这种物质可以在恒星的数十亿年寿命中存活下来，直到只剩下一颗被称为白矮星的炽热致密的残骸。白矮星的形成应该会“深度清洁”恒星附近的环境，但值得注意的是，我们已经发现了许多行星碎片的例子，在我们的研究中，我们的目标是找出这是如何发生的。还有许多其他白矮星是恒星演化留下的，我们将使用新一代光纤馈送光谱仪一次捕捉1000个物体来绘制这些白矮星的地图。

How do stars, planets and galaxies form? How do they evolve, how do they die? The Astronomy and Astrophysics group at the University of Warwick studies questions such as these through observations on telescopes, both large and small, and through physics-driven computational modelling. The use of optical telescopes in astronomy dates back over 400 years to Galileo, but we are now in a new Galilean era of discovery with the first detection of gravitational waves (GWs) only made in 2015. GWs provide a completely different view of the universe, delving to the heart of the most extreme events known as unimaginably dense stars spiral together, and, in their last moments before merging, rival the power output of the rest of the entire observable universe. GW telescopes can "see" almost everywhere at once, but have the equivalent of very blurred vision. To pinpoint sources, we need to see them electromagnetically (EM), i.e. with optical, radio and x-ray telescopes, but even that is difficult because you have to know where to look first. At Warwick we are working on a telescope called GOTO to do just this. From sites in Europe and Australia, GOTO is designed for breadth of vision and speed, to chase the universe's fastest and most violent events within minutes of their detection. Many less powerful, but longer lasting objects emit GWs much closer to Earth within our own galaxy, the Milky Way. We are starting to find systems from EM observations that will also be detectable as GW sources from space. These are exotic sources: one consists of two stars, each the size of the Earth but 100,000 times more massive, that circle each other in a little over five minutes. We will apply specialist high-speed cameras to their study, mounted on large optical telescopes, to probe how they evolve and important step in understanding how many of them there are, and how they came to be. Gravitational waves have given us new eyes on the universe, but new instruments and techniques do almost the same thing. In 1995 the first exoplanet was found through a particularly sensitive application of an old tool of astronomy called spectroscopy. Since then thousands of planets have been found in a bewildering variety of systems, many very different from our Solar System. At Warwick we have long pursued the discovery of exoplanets using both telescopes on Earth and in space, and will do so in this grant in order to understand processes that can destroy or erode planets when they are close to their host stars. Many known exoplanets are close to their host stars, but that is in part due to how we find them, so another strand of our research aims to push planetary detection to wider orbits, closer to those of our Solar system. Warwick has a strong interest in a new ESA-led space mission called PLATO which will provide a dramatic boost to this work. PLATO has a large field of view to allow it to pick up planets orbiting the brightest stars. These are key targets as they are close by, but above all they allow even more challenging application of spectroscopy, enough to allow us to probe the very composition of the planetary atmospheres. Earth and the other planets of the Solar system formed from a disk of material around the young Sun that lives on as the planets themselves but also "debris" in the form of comets, asteroids and dust. We aim to find evidence for similar structures around other stars, in particular from their dust as it scatters starlight. Such material can survive the several billion year lifetime of the star until just a hot dense remnant called a white dwarf remains. The formation of a white dwarf should "deep clean" the environment close to the star, and yet remarkably we have found many example of the planetary debris, and within our research we aim to find out how this can be. There are many other white dwarfs left from stellar evolution which we will map using a new generation of fibre-fed spectrographs that capture objects, 1000 at a time.