All articles tagged with #milkyway
An international X-ray spacecraft has discovered that the Milky Way's supermassive black hole, Sagittarius A*, experienced powerful flares over the past 1,000 years, revealing a violent history previously unknown, which could reshape our understanding of black hole evolution and their influence on galaxy formation.
Using AI and millions of simulations, astronomers discovered that the Milky Way's central black hole, Sagittarius A*, is spinning near its maximum speed, challenging existing theories about magnetic behaviors in accretion disks.
The podcast episode discusses the concept of galactic archaeology, which allows scientists to reconstruct the history of the Milky Way and the universe by analyzing data from various telescopes, both large and small. By examining different wavelengths of light and rare star species, researchers can piece together the galaxy's past, including its merger history. The episode highlights the contributions of smaller telescopes in this field, emphasizing their significant impact alongside major observatories.
Astronomers have discovered a globular cluster, VVV CL002, that is rapidly moving toward the Milky Way's center, which is dominated by powerful tidal forces and the supermassive black hole Sagittarius A*. This cluster is the closest known GC to the galactic center, with an orbit ranging from 619 to 3,400 light-years away. Its metallicity measurements suggest it is an old cluster, formed far from its current location. The study of VVV CL002 provides insights into the survival and migration mechanisms of globular clusters near the galactic center, although it is likely doomed to eventual destruction due to its trajectory towards this tumultuous region.
Astronomers have discovered that the Small Magellanic Cloud, a satellite galaxy of the Milky Way, is actually composed of two galaxies, one behind the other. Using the Australian Square Kilometre Array Pathfinder and ESA's Gaia spacecraft, researchers observed distinct movements and compositions in gas clouds and young stars, suggesting the presence of two separate stellar nurseries. This finding challenges previous perceptions of the Small Magellanic Cloud's structure and may lead to a reevaluation of its name and classification. The research, led by Claire Murray, awaits publication in The Astrophysical Journal.
Astronomers have discovered that the Small Magellanic Cloud, a satellite galaxy of the Milky Way, is actually two galaxies, one behind the other. Claire Murray's team used the Australian Square Kilometre Array Pathfinder and ESA's Gaia spacecraft to observe the movement of gas and young stars, revealing two distinct star-forming regions with different metal abundances and distances from Earth. This finding challenges previous notions of the Small Magellanic Cloud's structure and may lead to a renaming of the galaxy, as it could be two separate celestial objects. The research awaits publication in The Astrophysical Journal.
Astronomers have discovered that the Small Magellanic Cloud, a dwarf galaxy near the Milky Way, is actually two galaxies, one behind the other. Claire Murray's team used the Australian Square Kilometre Array Pathfinder and ESA's Gaia spacecraft to observe the movement of gas and young stars, revealing two distinct star-forming regions with different metal abundances and distances from Earth. This finding challenges previous perceptions of the Small Magellanic Cloud and suggests it may need to be reclassified if the two objects are indeed separate galaxies. The research is set to be published in The Astrophysical Journal and is currently available on arXiv.
Astronomers have discovered that the Small Magellanic Cloud, a dwarf galaxy near the Milky Way, may actually be two galaxies, one obscured behind the other. Using the Australian Square Kilometre Array Pathfinder and ESA's Gaia spacecraft, researchers observed distinct movements and compositions in two separate regions of star formation, suggesting the presence of two celestial objects with similar masses. This finding challenges the previous understanding of the Small Magellanic Cloud's structure and may lead to a reevaluation of its classification and name.
Astronomers using the Magellan Clay telescope have discovered that the globular cluster VVV CL002 is on a tight retrograde orbit and is falling towards the Milky Way's center. The cluster, located 23,800 light years away and discovered in 2011, has a high eccentricity orbit with perigalactocentric and apogalactocentric distances indicating it is well within the galactic bulge. The study, which also analyzed the cluster's chemical composition, suggests that VVV CL002 is an old cluster that was formed outside the central region and is now spiraling inward, likely to be destroyed in the future. Further observations could provide insights into the survival and migration of such clusters.