Deep imaging suggests isolated galaxy forms stars without signs of past mergers
Using the Two-meter Twin Telescope (TTT3), Spanish astronomers have conducted deep optical imaging of an isolated dwarf galaxy known as NGC 6789. Results of the new observations, presented November 10 on the arXiv preprint server, shed more light on the star formation process in this galaxy. Isolated but forming stars Discovered in 1883, NGC 6789 is a blue compact dwarf (BCD) galaxy located some 12 million light years away in the Local Void-a region of space with far fewer galaxies than its surroundings. However, despite its extreme isolation, NGC 6789 shows recent central star formation activity. Previous observations of NGC 6789 have found that approximately 4% of its total stellar mass—about 100 million solar masses-formed within the past 600 million years. It turned out that the central star-forming region of this galaxy is embedded within an apparently undisturbed, redder elliptical outer structure. One question remains unanswered Therefore, what still baffles scientists is ...