Modelling the RXTE light curve of η Carinae from a 3D SPH simulation of its binary wind collision

AT Okazaki, SP Owocki, CMP Russell… - Monthly Notices of the …, 2008 - academic.oup.com
The very massive star system η Carinae exhibits regular 5.54 yr (2024 d) period disruptive
events in wavebands ranging from the radio to X-ray. There is a growing consensus that …

Modeling the RXTE light curve of Carinae from a 3-D SPH simulation of its binary wind collision

AT Okazaki, SP Owocki, CM Russell… - Mon. Not. Roy. Astron …, 2008 - inspirehep.net
The very massive star system $\eta $ Carinae exhibits regular 5.54-year (2024-day) period
disruptive events in wavebands ranging from the radio to X-ray. There is a growing …

[PDF][PDF] Modeling the RXTE light curve of η Carinae from a 3-D SPH simulation of its binary wind collision

AT Okazaki, SP Owocki, CM Russell… - arXiv preprint arXiv …, 2008 - Citeseer
The very massive star system η Carinae exhibits regular 5.54-year (2024-day) period
disruptive events in wavebands ranging from the radio to X-ray. There is a growing …

Modelling the RXTE light curve of η Carinae from a 3D SPH simulation of its binary wind collision

AT Okazaki, SP Owocki, CMP Russell… - Monthly Notices of the …, 2008 - Wiley Online Library
The very massive star system η Carinae exhibits regular 5.54 yr (2024 d) period disruptive
events in wavebands ranging from the radio to X‐ray. There is a growing consensus that …

Modeling the RXTE light curve of Carinae from a 3-D SPH simulation of its binary wind collision

AT Okazaki, SP Owocki, CM Russell… - arXiv preprint arXiv …, 2008 - arxiv.org
The very massive star system $\eta $ Carinae exhibits regular 5.54-year (2024-day) period
disruptive events in wavebands ranging from the radio to X-ray. There is a growing …

[PDF][PDF] Modeling the RXTE light curve of η Carinae from a 3-D SPH simulation of its binary wind collision

AT Okazaki, SP Owocki, CM Russell, MF Corcoran - Orbit, 2008 - scholar.archive.org
The very massive star system η Carinae exhibits regular 5.54-year (2024-day) period
disruptive events in wavebands ranging from the radio to X-ray. There is a growing …

Modelling the RXTE light curve of η Carinae from a 3D SPH simulation of its binary wind collision

AT Okazaki, SP Owocki, CMP Russell… - Monthly Notices of the …, 2008 - cir.nii.ac.jp
抄録< jats: title> Abstract</jats: title>< jats: p> The very massive star system η Carinae
exhibits regular 5.54 yr (2024 d) period disruptive events in wavebands ranging from the …

[PDF][PDF] Modeling the RXTE light curve of η Carinae from a 3-D SPH simulation of its binary wind collision

AT Okazaki, SP Owocki, CM Russell, MF Corcoran - Orbit, 2008 - bartol.udel.edu
The very massive star system η Carinae exhibits regular 5.54-year (2024-day) period
disruptive events in wavebands ranging from the radio to X-ray. There is a growing …

Modeling the RXTE light curve of eta Carinae from a 3-D SPH simulation of its binary wind collision

AT Okazaki, SP Owocki, CM Russell, MF Corcoran - astroscu.unam.mx
The very massive star system eta Carinae exhibits regular 5.54-year (2024-day) period
disruptive events in wavebands ranging from the radio to X-ray. There is a growing …

[PDF][PDF] Modeling the RXTE light curve of η Carinae from a 3-D SPH simulation of its binary wind collision

AT Okazaki, SP Owocki, CM Russell… - arXiv preprint arXiv …, 2008 - academia.edu
The very massive star system η Carinae exhibits regular 5.54-year (2024-day) period
disruptive events in wavebands ranging from the radio to X-ray. There is a growing …