AAPOD2 Image Archives
ARP 159 and NGC 4725
ARP 159
ARP 159 is a striking pair of interacting galaxies located in the constellation of Lynx. This system features a peculiar, distorted structure resulting from the gravitational interactions between the galaxies. The larger galaxy exhibits a warped, elongated shape with prominent tidal tails, indicating a past collision or close encounter with its smaller companion. These interactions often trigger bursts of star formation, evident from the bright blue regions within ARP 159, where new stars are being born. This dynamic interplay provides astronomers with a valuable opportunity to study the effects of galactic mergers and the evolution of galaxies over cosmic timescales.
NGC 4725
NGC 4725 is a unique barred spiral galaxy situated in the constellation of Coma Berenices. Unlike typical spiral galaxies, NGC 4725 possesses a single, prominent spiral arm extending from a central bar structure. This distinctive feature makes it an object of interest in the study of galactic morphology and dynamics. The galaxy's core is bright and active, hosting regions of intense star formation. Additionally, NGC 4725 is known for its Seyfert 2 nucleus, indicating the presence of an active galactic nucleus powered by a supermassive black hole. This galaxy offers insights into the complex processes governing the formation and evolution of spiral structures and the role of central bars in galactic development.