PATT-linked grant for Warwick Astronomy & Astrophysics Group, April 2009 to March 2011

在生命的末期，恒星会进入三种可能的致密状态，即白矮星、中子星或黑洞。按照我们的标准，这三种物质的密度都令人难以置信，例如，密度是铅的几千倍。这类天体的许多例子都是已知的，它们往往远不是不活动的，因为它们可以与其他恒星如此紧密地配对，以至于我们可以看到气体从一颗恒星转移到致密天体的效果。在这样的过程中，气体可以被加热到数百万度，使这些物体成为高效的X射线源。此外，白矮星和中子星都可以表现出爆炸效应，因为物质在它们上面吸积成不可控的聚变，在几秒钟或几分钟内产生大量能量。我们的工作重点是试图理解这样的过程，以及我们所看到的各种物体是如何相互联系的。这笔赠款的目的是支持在地面望远镜上观察这些天体所需的旅行，在那里我们对材料撞击这些引人注目的天体时发生的高速过程进行观测。

At the end of their lives stars settle into one of three possible final compact states known as white dwarfs, neutron stars or black-holes. All three of these are incredibly dense by our standards, thousands of times denser than lead for instance. Many examples of such objects are known, and they are often far from being inactive as they can be so closely paired up with other stars than we can see the effects of gas transferring from one star to the compact object. In such a process the gas can be heated to many millions of degrees making these object efficient X-ray sources. Furthermore, both white dwarfs and neutron stars can show explosive effects as material accreting onto them sparks into uncontrollable fusion, generating vast amounts of energy within seconds or minutes. Our work centres on trying to understand such processes and how the various objects that we see relate to one another. The purpose of this grant is to support the travel needed to observe these objects on ground-based telescopes where we carry out observations of the high-speed processes that occur as material crashes onto these remarkable objects.