论文标题
X射线Novae H1743-322和GX339-4的光曲线的形态在2005 - 2019年爆发期间
Morphology of the Light Curves for the X-ray Novae H1743-322 and GX339-4 during their Outbursts in 2005-2019
论文作者
论文摘要
基于X射线Novae H1743-322（IGR J17464-3213）和GX339-4的X射线Novae H1743-322（IGR J17464-3213）的长期Swift和最高观察结果，我们研究了形态并将其X射线爆炸的光曲线分类。特别是，我们已经证实存在两种根本不同类型的爆发，即软的（S）和硬（H），并在源中揭示了它们的品种，即Ultrabright（u）和中级（i）。这些爆发的光曲线差异的特性和起源是根据截断的积聚磁盘模型讨论的。
Based on long-term SWIFT, RXTE, and MAXI observations of the X-ray novae H1743-322 (IGR J17464-3213) and GX339-4, we have investigated the morphology and classified the light curves of their X-ray outbursts. In particular, we have confirmed the existence of two radically different types of outbursts, soft (S) and hard (H), in both sources and revealed their varieties, ultrabright (U) and intermediate (I). The properties and origin of the differences in the light curves of these outbursts are discussed in terms of the truncated accretion disk model.
