84 citations · 511 across the 30 of their papers we have counts for
30 papers
The Walkaway Star HP Tau/G2: Evidence for a Stellar Merger
Bo Reipurth, J. Bally, P. Friberg +6
HP~Tau/G2 is a luminous, short-period, fast-rotating G-type weak-line T Tauri star with a large radius, an oblate shape with gravity-darkening, little circumstellar material, and c…
ODS: A self-reporting system for radio telescopes to coexist with adaptive satellite constellations
Bang D. Nhan, Christopher G. De Pree, Anthony Beasley +14
Low Earth orbit (LEO) satellite constellations bring broadband internet and cellular service to the most remote locations on the planet. Unfortunately, many of these locations also…
Bayesian sampling with BeAtlas, a grid of synthetic Be star spectra I. Recovering the fundamental parameters of αEri and βCMi
A. C. Rubio, A. C. Carciofi, P. Ticiani +14
Classical Be stars are fast rotating, near main sequence B-type stars. The rotation and the presence of circumstellar discs profoundly modify the observables of active Be stars. Ou…
The binary system of the spinning-top Be star Achernar
P. Kervella, S. Borgniet, A. Domiciano de Souza +16
Achernar, the closest and brightest classical Be star, presents rotational flattening, gravity darkening, occasional emission lines due to a gaseous disk, and an extended polar win…
Untangling magnetic massive star properties with linear polarization variability and the Analytic Dynamical Magnetosphere model
M. S. Munoz, G. A. Wade, D. M. Faes +2
Light scattered off particles can become linearly polarized. Stars surrounded by oblique, co-rotating envelopes are therefore expected to manifest periodic linear polarimetric vari…
A Multi-observing-technique Study of the Dynamical Evolution of the Viscous Disk around the Be Star CMa
Mohammad R. Ghoreyshi, Alex C. Carciofi, Carol E. Jones +3
The observed emission lines of Be stars originate from a circumstellar Keplerian disk that are generally well explained by the Viscous Decretion Disk model. In an earlier work we p…