Research news on Circumstellar shells

Circumstellar shells as a research area focus on the structure, composition, formation, and evolution of shell-like gas and dust envelopes surrounding stars at various evolutionary stages, particularly asymptotic giant branch (AGB) stars, red supergiants, and some massive stars. Studies integrate high-resolution spectroscopy, interferometry, millimeter/submillimeter observations, and radiative transfer and hydrodynamic modeling to characterize mass-loss processes, dust nucleation and growth, chemical enrichment, and interaction with the interstellar medium. This field also investigates shell morphologies (e.g., spherical, clumpy, or asymmetric), episodic or pulsation-driven mass loss, and the role of circumstellar shells in shaping planetary nebulae and contributing to galactic chemical evolution.

Hubble captures light show around rapidly dying star

This stunning image from NASA's Hubble Space Telescope reveals a dramatic interplay of light and shadow in the Egg Nebula, sculpted by freshly ejected stardust. Located approximately 1,000 light-years away in the constellation ...

Persistent shock wave around dead star puzzles astronomers

Gas and dust flowing from stars can, under the right conditions, clash with a star's surroundings and create a shock wave. Now, astronomers using the European Southern Observatory's Very Large Telescope (ESO's VLT) have imaged ...

The Tycho supernova's hidden secret

In November 1572, a brilliant new star appeared in the constellation Cassiopeia, shining so brightly that it was visible during the day. Danish astronomer Tycho Brahe carefully documented this celestial phenomenon, and the ...

Supergiant star's gigantic bubble surprises scientists

Astronomers have discovered a vast and expanding bubble of gas and dust surrounding a red supergiant star—the largest structure of its kind ever seen in the Milky Way. The bubble, which contains as much mass as the sun, ...

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