| Page 25 | Departamento de Física | Universidad de Santiago de Chile

Diving into the whirlpool. Understanding accretion in High-Mass X-ray Binaries with Vela X-1

Enviado por Valeria.salas en Jue, 01/11/2024 - 12:47

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Wind Roche lobe overflow in high-mass X-ray binaries-A possible mass-transfer mechanism for ultraluminous X-ray sources

Enviado por Valeria.salas en Jue, 01/11/2024 - 12:45

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Formation of wind-captured disks in supergiant X-ray binaries-Consequences for Vela X-1 and Cygnus X-1

Enviado por Valeria.salas en Jue, 01/11/2024 - 12:37

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Reduction of the maximum mass-loss rate of OH/IR stars due to unnoticed binary interaction

Enviado por Valeria.salas en Jue, 01/11/2024 - 12:30

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Variability in high‐mass X‐ray binaries

Enviado por Valeria.salas en Jue, 01/11/2024 - 12:29

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Vela X-1 as a laboratory for accretion in High-Mass X-ray Binaries

Enviado por Valeria.salas en Jue, 01/11/2024 - 12:24

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Wind morphology around cool evolved stars in binaries

Enviado por Valeria.salas en Jue, 01/11/2024 - 12:22

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Wind morphology around cool evolved stars in binaries-The case of slowly accelerating oxygen-rich outflows

Enviado por Valeria.salas en Jue, 01/11/2024 - 12:21

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Hybrid magnetic structures around spinning black holes connected to a surrounding accretion disk

Enviado por Valeria.salas en Jue, 01/11/2024 - 12:20

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Complex stellar winds from evolved stars

Enviado por Valeria.salas en Jue, 01/11/2024 - 11:55

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Diving into the whirlpool. Understanding accretion in High-Mass X-ray Binaries with Vela X-1

Wind Roche lobe overflow in high-mass X-ray binaries-A possible mass-transfer mechanism for ultraluminous X-ray sources

Formation of wind-captured disks in supergiant X-ray binaries-Consequences for Vela X-1 and Cygnus X-1

Reduction of the maximum mass-loss rate of OH/IR stars due to unnoticed binary interaction

Variability in high‐mass X‐ray binaries

Vela X-1 as a laboratory for accretion in High-Mass X-ray Binaries

Wind morphology around cool evolved stars in binaries

Wind morphology around cool evolved stars in binaries-The case of slowly accelerating oxygen-rich outflows

Hybrid magnetic structures around spinning black holes connected to a surrounding accretion disk

Complex stellar winds from evolved stars

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