2 papers
astro-ph.SR2026
MAGIC's interferometric diameters of Ophiuchi and CMa and comparison with asteroseismic modelling
K. Abe, J. Abhir, A. Abhishek +165
Cephei type stars are massive (M) and known to have several pulsation modes with periods typically of a few hours. Despite a better understanding of their physi…
astro-ph.SR2026
Multiplicity of Massive stars in the Milky Way (M3W). II. The brightest single O stars: variability and systemic velocities
J. Maíz Apellániz, E. Madero Fuentes, G. Holgado +9
(ABRIDGED) M3W studies the dynamical properties of massive stars in the solar vicinity, such as their systemic velocities, which are affected by variability effects: pulsations, li…