论文标题
与新生的黑洞低质量X射线二进制相关的超新星残留物
A supernova remnant associated with a nascent black hole low-mass X-ray binary
论文作者
论文摘要
当高质量恒星的核心崩溃到黑洞中时，能量释放出来，通常会为产生超新星残留物的爆炸供电。黑洞的可观察窗口有限，因此很少与超新星残留物相关。分析多通信器数据，我们表明Maxi J1535-571是在恒星爆炸中产生的黑洞，引起了Supernova Remnant G323.7-1.0，这是Black Hole低量X射线X射线二进制和Supernova Remnant的关联之间的第一种情况。鉴于这种联系，我们可以从建模中推断出祖细胞系统是一个近距离二进制的，其主要恒星的初始质量约为。 23-35个太阳能大块，伴侣恒星的巨大量降低了10倍。
Energy released when the core of a high-mass star collapses into a black hole often powers an explosion that creates a supernova remnant. Black holes have limited windows of observability, and consequently are rarely identified in association with supernova remnants. Analysing multi-messenger data, we show that MAXI J1535-571 is the black hole produced in the stellar explosion that gave rise to the supernova remnant G323.7-1.0, making it the first case of an association between a black hole low-mass X-ray binary and a supernova remnant. Given this connection, we can infer from our modelling that the progenitor system was a close binary whose primary star had an initial mass of approx. 23-35 solar masses with a companion star about 10 times less massive.
