`spiral-galaxies` Related Article Results

NGC 4395 is a low-luminosity, late-type spiral galaxy located in the constellation Canes Venatici. It is notable for hosting an active galactic nucleus of Seyfert 1 type at its core while lacking a prominent galactic bulge. Due to these characteristics, NGC 4395 is regarded as an important example for studying the formation and evolution of active galactic nuclei and the physical properties of low-mass black holes. Spiral Galaxy NGC 4395 (NOIRLAB) " image-element-format="right" image-source="htt