37 citations · 108 across the 5 of their papers we have counts for
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astro-ph.SR2017★ 37 cited
Stellar parameters and H line profile variability of Be stars in the BeSOS survey
C. Arcos, S. Kanaan, J. Chávez +3
The Be phenomenon is present in about 20 of the B-type stars. Be stars show variability on a broad range of timescales, which in most cases is related to the presence of a circ…
astro-ph.SR2017★ 8 cited
-Slow Solutions and Be Star Disks
I. Araya, C. E. Jones, M. Curé +4
As the disk formation mechanism(s) in Be stars is(are) as yet unknown, we investigate the role of rapidly rotating radiation-driven winds in this process. We implemented the effect…