activity
20012022
most citedFirst Light for GRAVITY: Phase Referencing Optical Interferometry for the Very Large Telescope Interferometer

588 citations · 1.8k across the 41 of their papers we have counts for

collaborators

41 papers

astro-ph.SR2022★ 8 cited

Trumpler 16-26: A New Centrifugal Magnetosphere Discovered via SDSS/APOGEE H-band Spectroscopy

S. Drew Chojnowski, Swetlana Hubrig, Jonathan Labadie-Bartz +6

We report the discovery of a new example of the rare class of highly magnetized, rapidly rotating, helium enhanced, early B stars that produce anomalously wide hydrogen emission du…

astro-ph.SR2022★ 3 cited

The outer orbit of the high-mass stellar triple system Herschel 36 determined with the VLTI

J. Sanchez-Bermudez, C. A. Hummel, J. Díaz-López +8

Multiplicity is a ubiquitous characteristic of massive stars. Multiple systems offer us a unique observational constraint on the formation of high-mass systems. Herschel 36 A is a…

astro-ph.SR2021★ 6 cited

Detection of anomalous element distribution in the extremely slowly rotating magnetic O9.7 V star HD 54879

S. P. Järvinen, S. Hubrig., M. Schöller +4

The O9.7 V star HD 54879 is currently the only massive magnetic star whose magnetic field geometry and rotation period are not constrained. Over the last three years, we gathered a…

astro-ph.SR2021★ 11 cited

Dynamical parallax, physical parameters and evolutionary status of the components of the bright eclipsing binary α Draconis

K. Pavlovski, C. A. Hummel, A. Tkachenko +13

Altough both components of the bright eclipsing binary Dra having been resolved using long baseline interferometry and the secondary component shown to contribute some 15\% of…

astro-ph.SR2021★ 21 cited

Surveying the Bright Stars by Optical Interferometry III: A Magnitude-Limited Multiplicity Survey of Classical Be-Stars

D. J. Hutter, C. Tycner, R. T. Zavala +3

We present the results of a multiplicity survey for a magnitude-limited sample of 31 classical Be stars conducted with the Navy Precision Optical Interferometer and the Mark III St…

astro-ph.EP2021★ 12 cited

First MATISSE L-band observations of HD 179218. Is the inner 10 au region rich in carbon dust particles?

E. Kokoulina, A. Matter, B. Lopez +58

Carbon is one of the most abundant components in the Universe. While silicates have been the main focus of solid phase studies in protoplanetary discs (PPDs), little is known about…