activity
20152020
most citedResolving the stellar activity of the Mira AB binary with ALMA

218 citations · 417 across the 5 of their papers we have counts for

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6 papers · 1 filter

astro-ph.SR202020 cited

ALMA and VLA reveal the lukewarm chromospheres of the nearby red supergiants Antares and Betelgeuse

E. O'Gorman, G. M. Harper, K. Ohnaka +8

We first present spatially resolved ALMA and VLA continuum observations of the early-M red supergiant Antares to search for the presence of a chromosphere at radio wavelengths. We…

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.SR201740 cited

The shock-heated atmosphere of an asymptotic giant branch star resolved by ALMA

Wouter Vlemmings, Theo Khouri, Eamon O'Gorman +8

Our current understanding of the chemistry and mass-loss processes in solar-like stars at the end of their evolution depends critically on the description of convection, pulsations…

astro-ph.SR201757 cited

An Updated 2017 Astrometric Solution for Betelgeuse

G. M. Harper, A. Brown, E. F. Guinan +4

We provide an update for the astrometric solution for the Type II supernova progenitor Betelgeuse using the revised Hipparcos Intermediate Astrometric Data (HIAD) of van Leeuwen, c…

astro-ph.SR2016

Study of the inner dust envelope and stellar photosphere of the AGB star R Doradus using SPHERE/ZIMPOL

T. Khouri, M. Maercker, L. B. F. M. Waters +12

We use high-angular-resolution images obtained with SPHERE/ZIMPOL to study the photosphere, the warm molecular layer, and the inner wind of the close-by oxygen-rich AGB star R Dora…

astro-ph.SR2015218 cited

Resolving the stellar activity of the Mira AB binary with ALMA

W. H. T. Vlemmings, S. Ramstedt, E. O'Gorman +4

We present the size, shape and flux densities at millimeter continuum wavelengths, based on ALMA science verification observations in Band 3 (~94.6 GHz) and Band 6 (~228.7 GHz), fr…