The H.E.S.S. telescope system has discovered three extremely luminous gamma-ray sources in the Large Magellanic…
Browsing: Large Magellanic Cloud
The Large Magellanic Cloud (LMC) is a satellite galaxy of the Milky Way, located approximately 163,000 light-years away from Earth. It is one of the closest galaxies to our own and is visible primarily from the Southern Hemisphere, appearing as a faint, cloud-like patch in the night sky. The LMC is classified as a dwarf irregular galaxy, though it shows signs of a bar structure, and it is less massive and organized than spiral galaxies like the Milky Way. This galaxy is an important site for astronomical research because it hosts a variety of astronomical phenomena that are relatively close by cosmic standards, making them easier to study. These include supernovae, star-forming regions, and the Tarantula Nebula—one of the most active and luminous star-forming regions in the local group of galaxies. The LMC also plays a crucial role in refining our understanding of stellar evolution and cosmology, particularly through the observation of Cepheid variable stars, which are used to measure cosmic distances.
This newly released Hubble image shows a small part of the Large Magellanic Cloud.…
A new ESO image explores the Large Magellanic Cloud and an area nicknamed the Dragon’s…
A new image from ESO’s Very Large Telescope reveals a closer look at NGC 2014…
By observing a rare close pair of stars, known as eclipsing binaries, a team of…
This Hubble Space Telescope image shows the Large Magellanic Cloud and the many star-forming regions…
Produced by Hubble’s Advanced Camera for Surveys, the above image is a close-up view of…
Using complex direct N-body simulations, scientists believe they solved the mystery of ultramassive stars of…
A new image from the NASA/ESA Hubble Space Telescope’s Wide Field Planetary Camera 2 shows…