Sudeshna Boro Saikia

TL;DR: In this paper, the average unsigned magnetic flux following an activity-rotation relation separating into saturated and unsaturated regimes was studied for stars that have been previously mapped with ZDI.

TL;DR: In this article, the authors considered whether non-dipolar field modes contribute significantly to the spin-down of low-mass stars and used a sample of stars that have all been previously mapped with Zeeman-Doppler imaging.

TL;DR: In this article, the average unsigned magnetic flux following an activity-rotation relation separating into saturated and unsaturated regimes was studied. And the authors showed that a power law relationship between the average photospheric magnetic flux recovered by ZDI, and that recovered by Zeeman broadening studies, can be found.

TL;DR: In this article, the authors considered whether non-dipolar field modes contribute significantly to the spin-down of low-mass stars and used a sample of stars that have all been previously mapped with Zeeman-Doppler imaging.

TL;DR: In this article , the adsorption of gallium onto chemical and biogenic elemental tellurium nanoparticles (BioTeNPs) was investigated and the experimental data fitted the monolayer adaption theory-based Langmuir model.