The Phoenix dwarf galaxy, discovered in 1976, was originally mistaken for a globular cluster. At a distance of 1.4 million light years from Earth, it is, in fact, a dwarf galaxy, but one that defies easy classification. According to the European Southern Observatory, it does not contain enough mass for build new stars, but a cloud of nearby gas, presumably ejected by supernova explosions, seems to suggest relatively recent star formation and the presence of relatively young suns. The gas does not reside within the galaxy, but it is gravitationally connected, indicating it eventually will fall back into the dwarf. This image was captured by ESO’s Very Large Telescope using the visual and near ultraviolet FOcal Reducer and low dispersion Spectrograph, or FORS2, instrument.
This NASA/ESA Hubble Space Telescope image captures the glow of distant stars within NGC 5264, a dwarf galaxy located just over 15 million light-years away in the constellation of Hydra (The Sea Serpent). NGC 5264 clearly possesses an irregular shape — unlike the more common spiral or elliptical galaxies — with knots of blue star formation.
The spectacular aftermath of a 360 million year old cosmic collision is revealed in great detail in new images from ESO’s Very Large Telescope. Among the debris is a rare and mysterious young dwarf galaxy. This galaxy is providing astronomers with an excellent opportunity to learn more about similar galaxies that are expected to be common in the early universe, but are normally too faint and distant to be observed by current telescopes.
A dwarf galaxy discovered close to the famous Sculptor Galaxy (NGC 253) by Australian astrophotographer Michael Sidonio has been studied in detail by the 8-metre Subaru Telescope in Hawaii. This fruitful collaboration between amateur and professional astronomers has revealed that the dwarf galaxy, now known as NGC 253-dw2, is being disrupted by the nearby giant spiral.