binaries:close相关论文
The first photometric analysis of V811 Cep was carried out.The first complete light curves of V,R and I bands are given.......
Data release 2 (DR2) from the Gaia mission was of great help in precise determination of fundamental parameters of Close......
I find that a (～) 0.1-1 M☉ outflowing equatorial dusty disk (torus) that the binary system progenitor of an intermediate......
The lander of Chinas Change 3 spacecraft was equipped with a 15-cm telescope that is used to monitor celestial objects i......
1FGL J1018.6–5856 is a high mass gamma-ray binary containing a compact object orbiting around a massive star with a per......
The deep and low-mass-ratio contact binary CSS J022914.4+044340 with a luminous additional companion
The first B-,V-,R_c-and I_c-band light curves of CSS J022914.4+044340 are presented and analyzed.It is found that CSS J0......
Data release 2(DR2) from the Gaia mission was of great help in precise determination of fundamental parameters of Close ......
The first photometric analysis of V811 Cep was carried out.The first complete light curves of V,R and I bands are given.......
Accretion induced collapse (AIC) may be responsible for the formation of some interesting neutron star binaries (e.g.,mi......
I find that a≃0.1−1M⊙outflowing equatorial dusty disk(torus)that the binary system progenitor of an intermediate lumi......
We apply the jet-powered ILOT scenario to two recently studied intermediate luminosity optical transients(ILOTs),and fin......
The new complete BVRcIc light curves and spectra of the short-period eclipsing binary XZ CMi are presented.The results f......
We performed a detailed photometric analysis of eight ultra-short period eclipsing binaries(USPEBs)using the Wilson-Devi......
Photometric study of eclipsing binaries in the Large Magellanic Cloud - I. W UMa type binaries in th
Eclipsing binaries are among the most important sources of information on stellar parameters like radii, masses, luminos......
We present photometric observations in Sloan filters g′, i′of the eclipsing W UMa stars USNOA2.0 1350-17365531, V471 C......
It has been suggested that Type Ia supernovae(SNe Ia) could be produced in the conditions of the violent merger scenario......
Four-color charge-coupled device(CCD) light curves in the B, V, Rc and I c bands of the totaleclipsing binary system V18......
Six mid-eclipse times of the eclipsing binary XZ And are obtained, which are analyzed together with others collected fro......
Accreting millisecond X-ray pulsars(AMXPs) are an important subclass of low-mass X-ray binaries(LMXBs), in which coheren......
