Supported by the National Natural Science Foundation of China.Acknowledgements This work was partly supported by the National Natural Science Foundation of China (Grant Nos. 11133007 and 11325315). Ne
We follow the premise that most intermediate luminosity optical transients(ILOTs) are powered by rapid mass accretion onto a main sequence star,and study the ef
Classical Newtonian f and g series for a Keplerian two-body problem are extended for the case of a post-Newtonian two-body problem with parameters β and γ. Th