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ATOMIUM: A high-resolution view on the highly asymmetric wind of the AGB star π1Gruis-I. First detection of a new companion and its effect on the inner wind

Enviado por Valeria.salas en Vie, 01/05/2024 - 13:37

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Leer más sobre ATOMIUM: A high-resolution view on the highly asymmetric wind of the AGB star π1Gruis-I. First detection of a new companion and its effect on the inner wind

ATOMIUM: The astounding complexity of the near circumstellar environment of the M-type AGB star R Hydrae-I. Morpho-kinematical interpretation of CO and SiO emission

Enviado por Valeria.salas en Vie, 01/05/2024 - 13:32

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Leer más sobre ATOMIUM: The astounding complexity of the near circumstellar environment of the M-type AGB star R Hydrae-I. Morpho-kinematical interpretation of CO and SiO emission

Revisiting the archetypical wind accretor Vela X-1 in depth-Case study of a well-known X-ray binary and the limits of our knowledge

Enviado por Valeria.salas en Vie, 01/05/2024 - 13:26

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Leer más sobre Revisiting the archetypical wind accretor Vela X-1 in depth-Case study of a well-known X-ray binary and the limits of our knowledge

X-ray emission from BH+ O star binaries expected to descend from the observed galactic WR+ O binaries

Enviado por Valeria.salas en Vie, 01/05/2024 - 13:25

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Leer más sobre X-ray emission from BH+ O star binaries expected to descend from the observed galactic WR+ O binaries

Radiation-hydrodynamics with MPI-AMRVAC-Flux-limited diffusion

Enviado por Valeria.salas en Vie, 01/05/2024 - 12:44

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ATOMIUM: ALMA tracing the origins of molecules in dust forming oxygen rich M-type stars-Motivation, sample, calibration, and initial results

Enviado por Valeria.salas en Vie, 01/05/2024 - 12:42

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Leer más sobre ATOMIUM: ALMA tracing the origins of molecules in dust forming oxygen rich M-type stars-Motivation, sample, calibration, and initial results

Binary-object spectral-synthesis in 3D (BOSS-3D)-Modelling Hα emission in the enigmatic multiple system LB-1

Enviado por Valeria.salas en Vie, 01/05/2024 - 12:39

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Leer más sobre Binary-object spectral-synthesis in 3D (BOSS-3D)-Modelling Hα emission in the enigmatic multiple system LB-1

Spinning black holes magnetically connected to a Keplerian disk-Magnetosphere, reconnection sheet, particle acceleration, and coronal heating

Enviado por Valeria.salas en Vie, 01/05/2024 - 12:38

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Leer más sobre Spinning black holes magnetically connected to a Keplerian disk-Magnetosphere, reconnection sheet, particle acceleration, and coronal heating

VizieR Online Data Catalog: Observational properties of the ATOMIUM project (Gottlieb+, 2022)

Enviado por Valeria.salas en Vie, 01/05/2024 - 12:36

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Leer más sobre VizieR Online Data Catalog: Observational properties of the ATOMIUM project (Gottlieb+, 2022)

First 3D radiation-hydrodynamic simulations of Wolf-Rayet winds

Enviado por Valeria.salas en Vie, 01/05/2024 - 12:34

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Leer más sobre First 3D radiation-hydrodynamic simulations of Wolf-Rayet winds

ATOMIUM: A high-resolution view on the highly asymmetric wind of the AGB star π1Gruis-I. First detection of a new companion and its effect on the inner wind

ATOMIUM: The astounding complexity of the near circumstellar environment of the M-type AGB star R Hydrae-I. Morpho-kinematical interpretation of CO and SiO emission

Revisiting the archetypical wind accretor Vela X-1 in depth-Case study of a well-known X-ray binary and the limits of our knowledge

X-ray emission from BH+ O star binaries expected to descend from the observed galactic WR+ O binaries

Radiation-hydrodynamics with MPI-AMRVAC-Flux-limited diffusion

ATOMIUM: ALMA tracing the origins of molecules in dust forming oxygen rich M-type stars-Motivation, sample, calibration, and initial results

Binary-object spectral-synthesis in 3D (BOSS-3D)-Modelling Hα emission in the enigmatic multiple system LB-1

Spinning black holes magnetically connected to a Keplerian disk-Magnetosphere, reconnection sheet, particle acceleration, and coronal heating

VizieR Online Data Catalog: Observational properties of the ATOMIUM project (Gottlieb+, 2022)

First 3D radiation-hydrodynamic simulations of Wolf-Rayet winds

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