Zobrazeno 1 - 10
of 1 405
pro vyhledávání: '"LI Xiang-dong"'
Autor:
Deng, Zhu-Ling, Li, Xiang-Dong
While there are over a dozen known neutron star (NS) symbiotic X-ray binaries (SyXBs) in the Galaxy, none SyXBs containing a black hole (BH) have been detected. We address this problem by incorporating binary population synthesis and the accretion pr
Externí odkaz:
http://arxiv.org/abs/2411.07548
We introduce the Langevin deformation for the R\'enyi entropy on the $L^2$-Wasserstein space over $\mathbb{R}^n$ or a Riemannian manifold, which interpolates between the porous medium equation and the Benamou-Brenier geodesic flow on the $L^2$-Wasser
Externí odkaz:
http://arxiv.org/abs/2410.20369
The discrepancies between observations and theoretical predictions of cataclysmic variables (CVs) suggest that there exists unknown angular momentum loss mechanism(s) besides magnetic braking and gravitational radiation. Mass loss due to nova eruptio
Externí odkaz:
http://arxiv.org/abs/2410.15254
Autor:
Chi, Yi-Heng, Huang, Jiahui, Zhou, Ping, Feng, Hua, Li, Xiang-Dong, Markoff, Sera B., Safi-Harb, Samar, Olivera-Nieto, Laura
How black holes are formed remains an open and fundamental question in Astrophysics. Despite theoretical predictions, it lacks observations to understand whether the black hole formation experiences a supernova explosion. Here we report the discovery
Externí odkaz:
http://arxiv.org/abs/2410.06510
Instability in supernova fallback disks and its effect on the formation of ultra long period pulsars
Several pulsars with unusually long periods were discovered recently, comprising a potential population of ultra long period pulsars (ULPPs). The origin of their long periodicity is not well understood, but may be related to magnatars spun down by su
Externí odkaz:
http://arxiv.org/abs/2410.05944
Autor:
Shao, Yi-Xuan, Zhou, Ping, Li, Xiang-Dong, Zhang, Bin-Bin, Castro-Tirado, Alberto Javier, Wang, Pei, Li, Di, Zhang, Zeng-Hua, Zhang, Zi-Jian, Hu, You-Dong, Pandey, Shashi B.
The Galactic magnetar SGR J1935+2154 has undergone another outburst since 2022 October 10. We present the results of searching for an optical/NIR counterpart of SGR J1935+2154 before and during this outburst. No counterpart was detected at the magnet
Externí odkaz:
http://arxiv.org/abs/2410.00635
Autor:
Gao, Shi-Jie, Shao, Yi-Xuan, Wang, Pei, Zhou, Ping, Li, Xiang-Dong, Zhang, Lei, Kania, Joseph W., Lorimer, Duncan R., Li, Di
Observations show that globular clusters might be among the best places to find millisecond pulsars. However, the globular cluster Terzan 6 seems to be an exception without any pulsar discovered, although its high stellar encounter rate suggests that
Externí odkaz:
http://arxiv.org/abs/2409.10801
Autor:
Yang, Hao-Ran, Li, Xiang-Dong
Swift J1858.6$-$0814 (hereafter J1858) is a transient neutron star low-mass X-ray binary (NS LMXB). There is controversy regarding its donor mass derived from observations and theoretical calculations. In this paper, we adopt seven magnetic braking (
Externí odkaz:
http://arxiv.org/abs/2409.05067
Autor:
Cui, Zhe, Li, Xiang-Dong
Millisecond pulsar + helium white dwarf (MSP+He WD) binaries are thought to have descended from neutron star (NS) low-mass X-ray binaries (LMXBs). The NSs accreted from the progenitors of the WDs and their spin periods were accordingly accelerated to
Externí odkaz:
http://arxiv.org/abs/2408.16561
IC 10 X-1 is one of close X-ray binaries containing a Wolf-Rayet donor, which can provide an evolutionary link between high-mass X-ray binaries and gravitational wave sources. It is still unclear about the precise nature of the accreting compact obje
Externí odkaz:
http://arxiv.org/abs/2408.08004