Recent simulations of Be stars in misaligned binary systems have revealed that misalignment between the disc and binary orbit can cause the disc to undergo Kozai–Lidov …
Context. The initial distribution of rotational velocities of stars is still poorly known, and how the stellar spin evolves from birth to the various end points of stellar evolution is an actively …
RG Rast, CE Jones, AC Carciofi… - The Astrophysical …, 2024 - iopscience.iop.org
We examine the evolution of the disk surrounding the Be star in the highly eccentric 10.8 yr binary system δ Scorpii over its three most recent periastron passages. V-band and B− V …
M Agarwal, P Aggarwal, G Sunil… - … (OTCON) on Smart …, 2024 - ieeexplore.ieee.org
The abstract of this research paper encapsulates the essence of a comprehensive investigation into stellar classification using linear regression. The study explores the …
COCAC Carciofi, ME Oksala, A David-Uraz, R Klement… - iau.org
1. Background The Working Group on Active B Stars (WGABS, formerly Working Group on Be Stars) was re-established under IAU Commission No. 29 in 1979 to promote and …