Page 3: Research news on Circumstellar disks

Circumstellar disks as a research area encompasses the observational, theoretical, and computational study of gas and dust structures surrounding young and evolved stars, with emphasis on their formation, dynamics, composition, and role in planet formation and mass-loss processes. This field integrates high-resolution imaging, spectroscopy, radiative transfer modeling, and magnetohydrodynamics to investigate protoplanetary and debris disks, disk accretion and winds, dust growth and migration, and disk-planet interactions. Research also addresses disk chemistry, ionization and thermal structure, and the coupling of disks to stellar magnetic fields, linking star formation, early stellar evolution, and the emergence of planetary systems.

Planet-forming disks lose gas faster than dust, new survey finds

An international team of astronomers including researchers at the University of Arizona Lunar and Planetary Laboratory has unveiled groundbreaking findings about the disks of gas and dust surrounding nearby young stars, using ...

Silicate clouds discovered in atmosphere of distant exoplanet

Astrophysicists have gained precious new insights into how distant exoplanets form and what their atmospheres can look like, after using the James Webb Telescope to image two young exoplanets in extraordinary detail. Among ...

Disk discovery changes views on star and planet formation

A study led by Paolo Padoan, ICREA research professor at the Institute of Cosmos Sciences of the University of Barcelona (ICCUB), is challenging the understanding of planetary disk formation around young stars.

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