Best Tucana
E0102, formally designated 1E 0102.2-7219, is a young, oxygen-rich supernova remnant located in the Small Magellanic Cloud, a dwarf galaxy orbiting the Milky Way. Estimated to be approximately 2,000 years old, it is the brightest X-ray source in its host galaxy and has been extensively studied by in...
1E 0102.2-7219 is an oxygen-rich supernova remnant located in the Small Magellanic Cloud, a satellite galaxy of the Milky Way. It is one of the few known oxygen-rich remnants in a galaxy outside our own, making it valuable for studies of stellar nucleosynthesis and supernova physics. The expanding e...
E0102-72.3 is a young, oxygen-rich supernova remnant located in the Small Magellanic Cloud, a dwarf galaxy orbiting the Milky Way. It is the result of a massive star's core collapse that occurred roughly 2,000 years ago as observed from Earth. The remnant is scientifically significant because its ex...
N90 is an H II region and star-forming nebula located within the Small Magellanic Cloud, a dwarf galaxy near the Milky Way. It surrounds the young open cluster NGC 602, which is actively shaping the surrounding interstellar medium. Radiation and stellar winds from the cluster's hot young stars have...
N90 is a large star-forming nebular complex in the Small Magellanic Cloud, a satellite galaxy of the Milky Way in the constellation Tucana. It contains the young open cluster NGC 602, whose hot, massive stars emit radiation and stellar winds that ionize and reshape the surrounding gas and dust. Imag...
N76 is a Wolf-Rayet nebula and H II region in the Small Magellanic Cloud, centered on the Wolf-Rayet binary system AB7. Its gas is ionized by the hot central stellar source, while stellar winds have produced a hot, relatively empty cavity inside the surrounding nebula. Astronomical studies model N76...
