All articles tagged with #sombrero galaxy
The James Webb Space Telescope captured its most detailed image yet of the Sombrero Galaxy, revealing new features such as interstellar dust clouds and red giant stars, enhancing our understanding of this peculiar galaxy's structure and history.
NASA's James Webb Space Telescope has captured detailed near-infrared images of the Sombrero Galaxy, revealing its dense star bulge, dust lanes, and evidence of a turbulent past involving galaxy mergers, while also showcasing individual stars and distant galaxies in unprecedented detail.
NASA's James Webb Space Telescope has captured new near-infrared images of the Sombrero Galaxy, revealing details about its core, dust, and past mergers, enhancing our understanding of galaxy evolution.
The James Webb Space Telescope has provided a new perspective on the Sombrero galaxy, revealing its smooth inner disk and complex outer ring through mid-infrared imaging. This view contrasts with the visible light images from the Hubble Space Telescope, which highlight the galaxy's glowing core. The new imagery suggests the presence of star-forming regions and reveals carbon-containing molecules in the dust ring. Despite its quiet star formation activity, the Sombrero galaxy hosts a supermassive black hole and numerous globular clusters, offering rich opportunities for astronomical study.
NASA's James Webb Space Telescope has captured a detailed mid-infrared image of the Sombrero Galaxy, revealing a clumpy dust structure in its outer ring, unlike the smooth appearance seen in previous observations. This new perspective highlights the distribution of dust, a key component in star formation, although the Sombrero Galaxy is not a major site for star creation. The galaxy, located 30 million light-years away in Virgo, also hosts a supermassive black hole and numerous globular clusters, offering rich opportunities for astronomical study.
The James Webb Space Telescope (JWST) has provided new insights into the Sombrero galaxy, revealing its outer dust ring as turbulent and clumpy, and highlighting a sparse, dust-depleted inner disk. The galaxy, which combines features of both spiral and elliptical galaxies, contains a supermassive black hole and forms only one solar mass of new stars annually. JWST's advanced capabilities have unveiled details previously unseen, including numerous background galaxies, suggesting the Sombrero galaxy may represent a galactic end-state after consuming its neighbors.
The James Webb Space Telescope (JWST) has captured a new image of the Sombrero Galaxy, revealing its dust rings in unprecedented detail at mid-infrared wavelengths. This view highlights clumps in the outer ring, suggesting young star-forming regions, despite the galaxy's low star production rate compared to others like the Cigar Galaxy. The image also showcases a backdrop of distant galaxies, underscoring JWST's role in advancing astronomical research. Demand for JWST observation time is high, with a nine-to-one oversubscription rate for upcoming cycles.
NASA's James Webb Space Telescope has captured a detailed mid-infrared image of the Sombrero galaxy, revealing clumpy dust in its outer ring and multiple inner rings, which were not visible in previous images by the Hubble and Spitzer telescopes. This new view provides insights into the galaxy's structure and star-forming regions, despite its relatively low star formation rate and inactive supermassive black hole.
The James Webb Space Telescope has captured a new image of the Sombrero Galaxy, revealing unexpected details. Unlike previous images from the Hubble Telescope, the JWST's Mid-Infrared Instrument shows that the galaxy's dust ring is not a significant site for star formation, and the central region features a flat disk rather than a halo of stars. The galaxy's active black hole is also less luminous than anticipated. These findings suggest the Sombrero Galaxy is more unusual than previously thought, with future studies likely focusing on its numerous globular clusters.
The James Webb Space Telescope has captured a new mid-infrared image of the Sombrero Galaxy, revealing its bright central core and intricate dust clumps in the outer ring, which may indicate young star formation. Unlike previous visible light images from the Hubble Space Telescope, Webb's view penetrates the galaxy's dusty center, showcasing the supermassive black hole at its core. This discovery provides astronomers with new insights into cosmic dust distribution and star formation in the Universe.
The James Webb Space Telescope's new mid-infrared image of the Sombrero Galaxy reveals a dust-rich outer ring and a quiet supermassive black hole, indicating the galaxy's star-forming days are nearly over. Despite its massive size, the Sombrero forms stars at a slower rate than the Milky Way due to a past starburst event that depleted its molecular hydrogen. The galaxy's isolation and lack of recent galactic interactions have left its central black hole inactive, marking a quiet phase in its evolution.
The James Webb Space Telescope has captured a new mid-infrared image of the Sombrero Galaxy, revealing a smooth inner disk and intricate clumps in its outer ring. These clumps, detected by Webb's MIRI, indicate young star-forming regions, although the galaxy itself is not a major site of star formation. The Sombrero Galaxy, located 30 million light-years away, contains a docile supermassive black hole and around 2000 globular clusters. The image also shows various background galaxies, providing insights into their properties.
NASA's Hubble Space Telescope has captured a breathtaking image of the Sombrero galaxy, located 28 million light-years away on the southern edge of the Virgo cluster. The image shows the galaxy in visible light, revealing its 50,000 light-year diameter and a central black hole estimated to be a billion times more massive than the Sun. The left and right edges of the galaxy appear red, the middle of the rings yellow-green, and the center light blue with a white core.
An astronomer in Spain has discovered a new active galaxy, tentatively named the Iris Galaxy, within the Sombrero Galaxy by analyzing images from the Hubble Space Telescope. The Iris Galaxy appears to have two spiral arms and may possess an active galactic nucleus (AGN) at its center, indicating the presence of star formation or a supermassive black hole. If the Iris Galaxy is bound to the Sombrero Galaxy's gravity, it would be a small galaxy around 1,000 light-years in size. However, if it is not bound, it could be much larger and located around 65 million light-years away.
Spanish astronomer Elio Quiroga Rodriguez has discovered a peculiar object in the Sombrero Galaxy, identified as a galaxy hosting an active galactic nucleus (AGN). By analyzing Hubble Space Telescope images, Rodriguez found that the object, previously classified as a globular cluster candidate, may be a barred spiral galaxy with an AGN at its center. The newfound galaxy, cataloged as PSO J190.0326-11.6132, has a radial velocity suggesting it could be a satellite of the Sombrero Galaxy. Further observations are needed to determine the type of AGN present in the galaxy.