Page 5: Research news on Accretion

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.

Not all Hot Jupiters orbit solo, observations suggest

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 ...

Planets can form in even the harshest conditions

According to the most widely held astronomical model (the nebular hypothesis), new stars are born from massive clouds of dust and gas (aka a nebula) that experience gravitational collapse. The remaining dust and gas form ...

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