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Variations of the high-level Balmer line spectrum of the helium-strong star Sigma Orionis E
Myron A. Smith, David A Bohlender
Using the high-level Balmer lines and continuum, we trace the density structure of two magnetospheric disk segments of the prototypical Bp star sigma Ori E (B2p) as these segments…
Variations of the ultraviolet resonance lines of the Be IV-V star zeta Cassiopeiae
Myron A. Smith, David A. Bohlender
Recently Neiner et al. reported that the B2 IV-V star zeta Cas contains a weak magnetic field which varies on the same 5.37 day period found from the modulations of its N V, C IV,…
On the X-ray and optical properties of the Be star HD 110432: a very hard-thermal X-ray emitter
Raimundo Lopes de Oliveira, Christian Motch, Myron A. Smith +3
(ABRIDGED) - HD 110432 is the first proposed, and best studied, member of a growing group of Be stars with X-ray properties similar to gamma Cas. These stars exhibit hard-thermal X…