论文标题
GX 339-4中Q图的研究
Study of the q diagram in GX 339-4
论文作者
论文摘要
黑洞X射线二进制（BHXB）GX 339-4在我们银河系中已知的X射线二进制源中产生最常见的X射线爆发（每2-4年）。在这里，我们介绍了使用硬度强度图（HID）（即Q图）观察到GX 339-4的演变的研究。我们对国际空间站（ISS）上的全套X射线图像（Maxi）望远镜的监视器（ISS）观察到的两个来源的爆发进行了分析。
Black hole X-ray binary (BHXB) GX 339-4 produces the most frequent X-ray outbursts (every 2-4 years) among known X-ray binary sources in our galaxy. Here we present the study of the evolution of GX 339-4 over the years of observations using the Hardness Intensity Diagram (HID), i.e., the q diagram. We present an analysis of two outbursts of the source observed by the Monitor of All-sky X-ray Image (MAXI) telescope aboard the International Space Station (ISS).
