The Large Magellanic Cloud, a satellite galaxy of the Milky Way, is the home of spectacular star-forming regions featuring complex tapestries of bright emission nebulae, dark dust lanes and colourful supernova remnants. NGC 2035 is a case in point, a lesser known region of the LMC discovered by the Scottish astronomer James Dunlop in 1826. This view was captured by the European Southern Observatory’s Very Large Telescope, showing clouds where new stars are being born along with the remnants of a supernova explosion (left).
Each year, NASA’s Chandra X-ray Observatory helps celebrate American Archive Month by releasing a collection of images using X-ray data. Each of these six new images — representing just a small fraction of the treasures that reside in Chandra’s unique archive — also includes data from telescopes covering other parts of the electromagnetic spectrum, such as visible and infrared light.
This NASA/ESA Hubble Space Telescope image captures the remnants of a long-dead star. These rippling wisps of ionised gas, named DEM L316A, are the remains of an especially energetic Type Ia supernova located some 160,000 light-years away within one of the Milky Way’s closest galactic neighbours — the Large Magellanic Cloud (LMC).
Several thousand years ago, a star some 160,000 light-years away from us exploded, scattering stellar shrapnel across the sky. The aftermath of this Type Ia supernova is shown here in this striking image from the NASA/ESA Hubble Space Telescope. The exploding star was a white dwarf located in the Large Magellanic Cloud, a close neighbouring galaxy.