43 citations · 50 across the 2 of their papers we have counts for
2 papers
astro-ph.SR2024★ 7 cited
Classical Be stars
Thomas Rivinius, Robert Klement
Classical Be stars, the "e" standing for the presence of spectroscopic line emission, are main sequence stars of spectral type B that are able to form a gaseous disk in Keplerian m…
astro-ph.SR2012★ 43 cited
Probing the properties of Be star discs with spectroastrometry and NLTE radiative transfer modelling: beta CMi
H. E. Wheelwright, J. E. Bjorkman, R. D. Oudmaijer +3
While the presence of discs around classical Be stars is well established, their origin is still uncertain. To understand what processes result in the creation of these discs and h…