Using high-resolution 1665/1667 MHz OH line and continuum spectrum observational data from the European VLBI Network and the Multi-Element Radio Linked Interferometer Network, Antneh Gashaye, a Ph.D. student from the Xinjiang Astronomical Observatory of the Chinese Academy of Sciences, has mapped the OH MegaMaser emission in the ultra-luminous infrared galaxy IRAS 15250+3609, and revealed the nature and structure of the OH MegaMaser emission in the galaxy.