activity
20162024
most citedInterferometric detections of sdO companions orbiting three classical Be stars

33 citations · 66 across the 11 of their papers we have counts for

collaborators

8 papers

astro-ph.SR202133 cited

Interferometric detections of sdO companions orbiting three classical Be stars

R. Klement, G. H. Schaefer, D. R. Gies +17

Classical Be stars are possible products of close binary evolution, in which the mass donor becomes a hot, stripped O or B-type subdwarf (sdO/sdB), and the mass gainer spins up and…

astro-ph.SR201714 cited

A Spectroscopic Orbit for the late-type Be star CMi

Nick Dulaney, Noel D. Richardson, Cody J. Gerhartz +12

The late-type Be star CMi is remarkably stable compared to other Be stars that have been studied. This has led to a realistic model of the outflowing Be disk by Klement et al.…

astro-ph.SR20164 cited

Pulsations and outbursts in Be stars: Small differences - big impacts

D. Baade, Th. Rivinius, A. Pigulski +12

New high-cadence observations with BRITE covering many months confirm that coupled pairs of nonradial pulsation modes are widespread among early-type Be stars. With the difference…

astro-ph.SR2016

Radiative transfer on decretion discs of Be binaries

Despina Panoglou, Daniel M. Faes, Alex C. Carciofi +2

In this work we explore the effect of binarity in the decretion disc of Be stars, in order to explain their variability. To this aim, we performed smoothed particle hydrodynamics (…

astro-ph.SR20162 cited

Be Stars Seen by Space Photometry

Thomas Rivinius, Dietrich Baade, Alex C. Carciofi

Classical Be stars are introduced as object class and their particular potential for space based photometry is highlighted. A brief summary of the various types of variability obse…

astro-ph.SR2016

Difference frequencies of nonradial pulsation modes and repetitive outbursts in classical Be stars

D. Baade, Th. Rivinius, A. Pigulski +2

Space photometry has revealed rich pulsation spectra in classical Be stars. Often frequency pairs can be found that differ by nearly the frequency of a third genuine stellar variab…