We present simulation results on evolution development of orbital motion of short-period comets with the revolution period not exceeding 6–7 years, namely come
Using observations from the Michelson Doppler Imager(MDI) onboard Solar and Heliospheric Observatory(SOHO), we develop a computational algorithm to automaticall
We propose that sub-Keplerian accretion belts around stars might launch jets. The sub-Keplerian inflow does not form a rotationally supported accretion disk, bu