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20242026
most citedSimulations of facular magnetic fields on cool stars I: Main sequence stars with solar metallicity

3 citations · 3 across the 2 of their papers we have counts for

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astro-ph.SR2024

Sun-like stars produce superflares roughly once per century

Valeriy Vasilyev, Timo Reinhold, Alexander I. Shapiro +7

Stellar superflares are energetic outbursts of electromagnetic radiation, similar to solar flares but releasing more energy, up to erg on main sequence stars. It is unkno…

astro-ph.SR2024

Low-latitude magnetic flux emergence on rapidly rotating solar-type stars

Emre Işık, Sami K. Solanki, Robert H. Cameron +1

Besides a dense coverage of their high latitudes by starspots, rapidly rotating cool stars also display low-latitude spots in Doppler images, although generally with a lower covera…

astro-ph.SR2024

First Calculations of Starspot Spectra based on 3D Radiative Magnetohydrodynamics Simulations

H. N. Smitha, Alexander I. Shapiro, Veronika Witzke +6

Accurate calculations of starspot spectra are essential for multiple applications in astronomy. The current standard is to represent starspot spectra by spectra of stars that are c…

astro-ph.EP2024

Reliable Transmission Spectrum Extraction with a Three-Parameter Limb Darkening Law

Rosa E. Keers, Alexander I. Shapiro, Nadiia M. Kostogryz +7

Stellar limb darkening must be properly accounted for to accurately determine the radii of exoplanets at various wavelengths. The standard approach to address limb darkening involv…

astro-ph.SR2024

Stellar Surface Magnetic Fields Impact Limb Darkening

Nadiia M. Kostogryz, Alexander I. Shapiro, Veronika Witzke +8

Stars appear darker at their limbs than at their disk centers because at the limb we are viewing the higher and cooler layers of stellar photospheres. Limb darkening derived from s…