Research news on Stellar rotation

Stellar rotation as a research area investigates the angular momentum content and evolution of stars, its observational diagnostics, and its impact on stellar structure and environments. It encompasses measurement techniques such as line broadening, rotational modulation of photometric and spectroscopic signals, and asteroseismology, as well as modeling of internal differential rotation, angular momentum transport, and magnetic braking. The field examines rotation’s role in dynamo-driven magnetic activity, mass loss, mixing of chemical elements, and evolutionary pathways from pre-main-sequence phases to compact remnants, with implications for stellar populations, gyrochronology, and progenitors of phenomena such as gamma-ray bursts and gravitational-wave sources.

How do close binary stars form?

Our sun is a bit of an outlier in the general stellar population. We typically think of stars as being solitary wanderers throughout the galaxy. But roughly half of sun-like stars are locked in with more than one companion ...

Why stars spin down, or up, before they die

From birth to death, stars generally slow by 100 to 1,000 times their initial rotation rates; in other words, they "spin down." The sun's total angular momentum has declined as material is gradually blown off at the surface ...

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