Theo Khouri
Theo är forskare på avdelningen för astronomi och plasmafysik.
Visar 43 publikationer
An impressionist view of V Hydrae: When MATISSE paints asymmetric giant blobs
ATOMIUM: Molecular inventory of 17 oxygen-rich evolved stars observed with ALMA
Probing the dynamical and kinematical structures of detached shells around AGB stars
One month convection timescale on the surface of a giant evolved star
First detection of AIF line emission towards M-type AGB stars
First detection of AlF line emission towards M-type AGB stars
Observational identification of a sample of likely recent common-envelope events
Investigating dust properties in AGB wind-ISM interaction regions
ATOMIUM: halide molecules around the S-type AGB star W Aquilae
Heavy-element Rydberg transition line emission from the post-giant-evolution star HD 101584
Maser emission from the CO envelope of the asymptotic giant branch star W Hydrae
VLTI/PIONIER reveals the close environment of the evolved system HD 101584
Inner dusty envelope of the AGB stars W Hydrae, SW Virginis, and R Crateris using SPHERE/ZIMPOL
(Sub)stellar companions shape the winds of evolved stars
CO and HCN isotopologue ratios in the outflows of AGB stars
ALMA spectrum of the extreme OH/IR star OH 26.5+0.6
HD 101584: circumstellar characteristics and evolutionary status
Imaging the dust and the gas around Mira using ALMA and SPHERE/ZIMPOL
High-resolution observations of gas and dust around Mira using ALMA and SPHERE/ZIMPOL
CO envelope of the symbiotic star R Aquarii seen by ALMA
Rotation of the asymptotic giant branch star R Doradus
Properties of dust in the detached shells around U Antilae, DR Serpentis, and V644 Scorpii
The shock-heated atmosphere of an asymptotic giant branch star resolved by ALMA
Constraints on the H2O formation mechanism in the wind of carbon-rich AGB stars
Unraveling The Dust Formation Process In R DOR
Detection of Rotational Co Emission from the Red-Supergiants in the Large Magellanic Cloud
ALMA Observations of Anisotropic Dust Mass Loss around VY CMa
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