activity
20152019
most citedThe close circumstellar environment of Betelgeuse - V. Rotation velocity and molecular envelope properties from ALMA

82 citations · 189 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR201928 cited

NOEMA maps the CO environment of the red supergiant Cep

M. Montargès, W. Homan, D. Keller +8

Red supergiant stars are surrounded by a gaseous and dusty circumstellar environment created by their mass loss which spreads heavy elements into the interstellar medium. The struc…

astro-ph.SR201782 cited

The close circumstellar environment of Betelgeuse - V. Rotation velocity and molecular envelope properties from ALMA

Pierre Kervella, Leen Decin, Anita M. S. Richards +6

We observed Betelgeuse using ALMA's extended configuration in band 7 (f~340 GHz, λ~0.88 mm), resulting in a very high angular resolution of 18 mas. Using a solid body rotation mode…

astro-ph.SR201711 cited

Radiation-pressure-driven sub-Keplerian rotation of the disc around the AGB star L2 Pup

Thomas J. Haworth, Richard A. Booth, Ward Homan +3

We study the sub-Keplerian rotation and dust content of the circumstellar material around the asymptotic giant branch (AGB) star L Puppis. We find that the thermal pressure gra…

astro-ph.SR201746 cited

Chemical content of the circumstellar envelope of the oxygen-rich AGB star R Dor: Non-LTE abundance analysis of CO, SiO, and HCN

M. Van de Sande, L. Decin, R. Lombaert +5

(abridged) Our aim is to determine the radial abundance profile of SiO and HCN throughout the stellar outflow of R Dor, an oxygen-rich AGB star with a low mass-loss rate. We have a…

astro-ph.SR201521 cited

Simplified models of stellar wind anatomy for interpreting high-resolution data: Analytical approach to embedded spiral geometries

Ward Homan, Leen Decin, Alex de Koter +3

Recent high-resolution observations have shown stellar winds to harbour complexities which strongly deviate from spherical symmetry, generally assumed as standard wind model. One s…

astro-ph.SR20151 cited

Gravity-mode period spacings as seismic diagnostic for a sample of gamma Doradus stars from Kepler space photometry and high-resolution ground-based spectroscopy

T. Van Reeth, A. Tkachenko, C. Aerts +20

Gamma Doradus stars (hereafter gamma Dor stars) are gravity-mode pulsators of spectral type A or F. Such modes probe the deep stellar interior, offering a detailed fingerprint of t…