"Adaptive Optics for Astronomy" is a specialized book that explores the revolutionary technology of adaptive optics in astronomy. This technology has enabled astronomers to overcome the limitations in image quality caused by atmospheric turbulence. Since the first observations in 1609, astronomers have tirelessly worked to improve the resolution of their instruments. Adaptive optics represents a significant advancement that allows for the breaking of resolution limits imposed by the Earth's atmosphere. The book highlights the development of this technology, the challenges it presents, and the opportunities it opens up for astronomy. It is aimed at professionals and students who wish to gain a deeper understanding of how adaptive optics works and its applications in modern astronomy.