BINARIES相关论文
We investigate the birthrate problem for low-mass X-ray binaries(LMXBs) and millisecond radio pulsars(MRPs) in this pape......
Based the Alfven wave oscillation model(AWOM) and relativistic precession model(RPM) for twin kHz QPOs,we estimate the e......
We construct a particle-number(n)-resolved master equation(ME) approach under the self-consistent Born approximation(SCB......
We present the observational results from a detailed timing analysis of the black hole candidate EXO 1846-031 during its......
为探究吕家坨井田地质构造格局,根据钻孔勘探资料,采用分形理论和趋势面分析方法,研究了井田7......
We present high-precision, multi-band CCD photometry of two less-studied close binaries V1123 Tau and V1128 Tau. Complet......
A likely candidate of type Ia supernova progenitors: the X-ray pulsating companion of the hot subdwa
HD49798 is a hydrogen depleted subdwarf 06 star and has an X-ray pulsating companion(RX J0648.0-4418).The X-ray pulsatin......
We present an XMM-Newton observation of the eclipsing binary Algol which contains an X-ray dark B8V primary and an X-ray......
A grid of binary evolution models are calculated for the study of a blue straggler (BS) population in intermediate age (......
We present the combined BVI multicolor photometric solutions of seven EW variables in the old open cluster Berkeley 39.T......
The new RS CVn binary V1034 Her revisited and the orbital period-activity relation of short-period R
This paper presents new CCD BV RI light curves of the newly discovered RS CVn eclipsing binary V1034 Her in 2009 and 201......
We present new charge-coupled device (CCD) photometry for the triple star EF Draconis,obtained in 2009 and 2011.Using th......
观测显示星系中的大部分恒星是双星，因此星族合成研究必须考虑双星的作用。综述双星对星族合成研究的重要性。主要讨论了双星对早型......
Most astrophysical accretion disks are likely to be warped.In X-ray binaries,the spin evolution of an accreting neutron ......
IO Cnc was classified to be a new G-type(G0)W UMa-type eclipsing binary system.Our first multicolor photometric solution......
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提出一种改进的运动目标检测算法,首先将视频序列中的一整幅画面进行分割,对分割产生的每块图像进行连续检测,一旦检测到有变化,即......
矮新星是爆发频繁的激变变星，主星是白矮星，次星是充满洛希瓣的晚型矮星；白矮星周围有吸积盘，物质流与吸积盘的碰撞区域即热斑。与大多......
天鹰座X-1(Aquila X-1,Aql X-1)是一个低质量中子星X射线双星,在X射线和射电波段表现为暂现源。对该源的甚长基线干涉(very long b......
化学组成特殊星（即CP星）是一类具有特殊化学元素丰度的恒星,大部分属于A型和B型主序星。主要介绍了CP星的分类、特征以及主要的起源......
CCD photometric observations of the short-period eclipsing binary DZ Lyn were obtained during seven nights in March-Apri......
We study non-thermal emissions from cascade processes in accreting X-raybinary pulsars. In the framework of the magnetos......
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早期的地面观测积累了大量关于双星系统的观测资料．相对于近年来的各种观测数据，这些资料兼有精度低的缺陷和时间跨度长的优势．针对同......
We present the orbits of ten visual binary stars: WDS 01015+6922, WDS 01424– 0645, WDS 01461+6349, WDS 04374–0951, WDS......
我们短时期的 W UMa 类型的电荷耦合器件光度计的观察的现在的结果联系二进制系统， RZ Com。二进制代码的轻曲线从 1998 ～ 2003 从 W......
Assuming a naive star formation history, we construct synthetic X-ray source pop- ulations, using a population synthesis......
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A likely candidate of type Ia supernova progenitors： the X-ray pulsating companion of the hot subdwa
HD 49798 is a hydrogen depleted subdwarf O6 star and has an X-ray pulsating companion (RX J0648.0-4418). The X-ray pulsa......
我们在场短时期的超越二进制代码的长期的解决时间的光度学 IU 每。它证实系统的内在的 δ 象 Scuti 一样跳动由 Kim 等报导了......
超越二进制代码的算法语言类型的轨道的时期变化， VW Hydrae，基于一最新坚定的日蚀时间和从文学收集的轻最小的另外的时间被分析。轨......
A grid of binary evolution models are calculated for the study of a blue straggler(BS) population in intermediate age(lo......
Seven charge-coupled device(CCD) photometric times of light minimum of the overcontact binary BS Cas which were obtained......
We present the photometric solutions of the variable star V30 that is in the foreground of intermediate open cluster NGC......
The multicolor photometric observations of the neglected eclipsing binary FT Ursae Majoris (FT UMa) were obtained in 201......
When observing blazars, we identified a new eclipsing binary named GSC03517–00663. The light curves of GSC 03517–00663......
We report the results of a search for variable stars in the open cluster NGC 2141. Ten variable stars are detected, amon......
Some properties of mass transfer within a semi-detached binary system are discussed based on an example of VV Vir.The ob......
HD 6840 is a double-lined visual binary with an orbital period of ～7.5 years. By fitting the speckle interferometric meas......
We present the complete set of physical and geometrical parameters of the visual close binary system GJ 9830 for the fir......
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The secular effect of gravitational radiation damping on the periastronadvance of binary stars in se
The second order perturbation effect of gravitational radiation damping on the periastronadvance of binary stars is stud......
By analyzing two sets of complete BV Rc Ic light curves for V342 UMa and three sets of complete BV Rc Ic light curves fo......
PSR B1259-63is a γ-ray emitting high mass X-ray binary system,in which the compact object is a millisecond pulsar.The s......
Meta-analysis of electron cyclotron resonance absorption features detected in high-mass X-ray binari
Using recent compilations of detailed X-ray observations and spectral models of exceptional quality, we record the elect......
