Stars:evolution相关论文
To investigate the effects of massive star evolution on surrounding molecules,we select nine massive clumps previously o......
Multi-band photometry and light curve analysis for two newly recognized contact binary systems,TYC 6995-813-1 and NSVS 1......
PSR J1946 + 3417 is a millisecond pulsar (MSP) with a spin period P ≈ 3.17 ms.Harbored in a binary with an orbital peri......
The first photometric analysis of V811 Cep was carried out.The first complete light curves of V,R and I bands are given.......
A cycle to cycle light variation of W UMa contact binary VW Cep revealed by the Lunar-Based Ultravio
W UMa contact binaries contain two late-type main-sequence stars where both components are filling the critical Roche lo......
The lander of Chinas Change 3 spacecraft was equipped with a 15-cm telescope that is used to monitor celestial objects i......
The first photometric analysis of V811 Cep was carried out.The first complete light curves of V,R and I bands are given.......
To investigate the effects of massive star evolution on surrounding molecules,we select nine massive clumps previously o......
The photometric and spectroscopic data for three double-lined detached eclipsing binaries were collected from the photom......
Accretion induced collapse (AIC) may be responsible for the formation of some interesting neutron star binaries (e.g.,mi......
Binary interactions lead to the formation of intriguing objects, such as compact binaries, super-novae, gamma ray bursts......
The first charge-coupled device photometric light curves in B,V,Rc,and Ic bands of the short-period contact binary star ......
The accretion-induced collapse(AIC)scenario was proposed 40 years ago as an evolutionary end state of oxygen-neon white ......
We performed a detailed photometric analysis of eight ultra-short period eclipsing binaries(USPEBs)using the Wilson-Devi......
The photometric and spectroscopic data for three double-lined detached eclipsing binaries were collected from the photom......
It has been suggested that Type Ia supernovae(SNe Ia) could be produced in the conditions of the violent merger scenario......
Accreting millisecond X-ray pulsars(AMXPs) are an important subclass of low-mass X-ray binaries(LMXBs), in which coheren......
使用不同的恒星辐射不透明度数值 ,对 5至 9个太阳质量恒星的演化模型进行计算 ,来研究辐射不透明度对赫罗图中蓝回绕的影响。结果......
大质量恒星由于其高光度、短寿命和质量损失 ,对星系的积分光谱能量分布和重元素增丰起主导作用 ,从而在研究星系的形成和演化上具......
Neutrinos play an important role in stellar evolution.They are produced by nuclear reactions or thermal processes.Using ......
Type Ia supernovae(SNe Ia)are thermonuclear explosions of carbon-oxygen white dwarfs(CO WDs),and are believed to be exce......
