Accretion as a research area investigates the physical processes by which diffuse material gravitationally aggregates to form larger astrophysical structures, including planets, stars, black holes, and galaxies. It encompasses the study of accretion disks, angular momentum transport, magnetohydrodynamic instabilities, radiative transfer, and the interplay between accretion flows and outflows or jets. This field integrates analytical theory, numerical simulations, and multiwavelength observations to quantify mass accretion rates, efficiency of gravitational energy conversion into radiation, and feedback on the surrounding medium, thereby constraining models of structure formation, compact object growth, and high-energy phenomena in various cosmic environments.
At the center of most large galaxies, including our own Milky Way, sits a supermassive black hole. Interstellar gas periodically falls into the orbit of these bottomless pits, switching the black hole into active galactic ...
Astronomy
Mar 17, 2025
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Rotating black holes are the most powerful phenomenon in the known universe. Their powerful gravity radically alters the curvature of spacetime around them, leading to relativistic effects like time dilation, light distortion, ...
Astronomy
Mar 10, 2025
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A fresh look at past data reveals that exoplanets with masses similar to Jupiter formed much sooner than previously thought, according to new research. The Ohio State University study's results provide new information about ...
Planetary Sciences
Mar 5, 2025
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A recent study published in The Astrophysical Journal has introduced a new theoretical model that explains astrophysical outflow phenomena spanning 12 orders of magnitude, from protostars to supermassive black holes.
Astronomy
Feb 24, 2025
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Black holes have been fascinating subjects of study, not just because they are cosmic vacuum cleaners, but also as engines of immense power capable of extracting and redistributing energy on a staggering scale. These dark ...
Astronomy
Feb 19, 2025
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A pair of astrophysicists with Aix- Marseille Université, CNRS, and Institut Universitaire de France have developed a new theory about the formation of Jupiter's largest moons. In their paper published in The Planetary Science ...
Planets are formed when dust and rock in a disk around a young star collide and combine to form ever larger bodies. This so-called accretion is not yet fully understood. Astrophysicists at the University of Duisburg-Essen ...
Astronomy
Jan 22, 2025
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Using observations from 2017 and 2018, the Event Horizon Telescope (EHT) Collaboration has advanced our understanding of the supermassive black hole at the center of Messier 87 (M87*). This study marks a significant step ...
Astronomy
Jan 22, 2025
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Active galactic nuclei are supermassive black holes at the center of certain galaxies. As matter falls into these black holes, enormous amounts of energy are released, making active galactic nuclei, or AGN, one of the most ...
Astronomy
Jan 17, 2025
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281
Hot Jupiters are giant planets initially known to orbit alone close to their star. During their migration towards their star, these planets were thought to accrete or eject any other planets present. However, this paradigm ...
Planetary Sciences
Jan 15, 2025
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