The youngest X-ray binaries
作者：Xiang-Dong Li
摘要：Several X-ray binaries(XRBs)have been identified to be associated with supernova remnants(SNRs).Because of the short lifetimes of SNRs,this leaves them to be the youngest known XRBs.This small group of binaries provides valuable information on the formation of compact stars under the framework of massive binary evolution.In this paper we review the observational characteristics of these youngest XRBs and discuss their possible implications on the initial conditions of compact stars and their interaction with the companion stars.
發文機構：School of Astronomy and Space Science Key Laboratory of Modern Astronomy and Astrophysics（Nanjing University）
關鍵詞：accretionaccretiondisksstars:blackholesstars:neutronevolution
分類號： P172.2[天文地球—天文學]
CSCD- The evolutionary status of chemically peculiar eclipsing binary star DV Boo
- The relaxation of galaxy clusters at redshift z=0 in IllustrisTNG simulation
- Radiative hydrodynamic simulations of the spectral characteristics of solar white-light flares
- Investigating the relationship between cosmic curvature and dark energy models with the latest supernova sample
- Astronomical Site Monitoring System at Lijiang Observatory
- A polarization study of the supernova remnant CTB 80
- Imaging atmospheric turbulence,using entropy to quantify turbulence strength
- The first results of observations of lunar occultations in different spectral ranges at the 6-m telescope of the SAO RAS
- The timing residual patterns due to pulsar acceleration
- Contact binaries at different evolutionary stages