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ON THE INTERACTION OF JETS WITH STELLAR WINDS IN MASSIVE X–RAY BINARIES.

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Title: ON THE INTERACTION OF JETS WITH STELLAR WINDS IN MASSIVE X–RAY BINARIES.
Authors: PERUCHO, MANEL1 manel.perucho@uv.es, BOSCH-RAMON, VALENTÍ2 vbosch@mpi-hd.mpg.de, KHANGULYAN, DMITRY2 Dmitry.Khangulyan@mpi-hd.mpg.de
Source: International Journal of Modern Physics D: Gravitation, Astrophysics & Cosmology. Jun2010, Vol. 19 Issue 6, p791-796. 6p. 4 Color Photographs.
Subjects: Stellar winds, X-ray binaries, Astronomy, Computer simulation, Space plasmas
Abstract: We present the first three-dimensional simulations of the evolution of a microquasar jet inside the binary star system. The aim is to study the interaction of these jets with the stellar wind from a massive companion and the possible locations of high-energy emission sites. We have simulated two jets with different injection power in order to give a hint on the minimum power required for the jet to escape the system and become visible in larger scales. In the setup, we include a massive star wind filling the grid through which the jet evolves. We show that jets should have powers of the order of 1037 erg s-1 or more in order not to be destroyed by the stellar wind. The jet–wind interaction results in regions in which high-energy emission could be produced. These results imply the possible existence of a population of X–ray binaries undetected in the radio band due to jet disruption inside the region dominated by the stellar wind. [ABSTRACT FROM AUTHOR]
Copyright of International Journal of Modern Physics D: Gravitation, Astrophysics & Cosmology is the property of World Scientific Publishing Company and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)
Database: Engineering Source
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DbLabel: Engineering Source
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  Data: ON THE INTERACTION OF JETS WITH STELLAR WINDS IN MASSIVE X–RAY BINARIES.
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  Data: <searchLink fieldCode="DE" term="%22Stellar+winds%22">Stellar winds</searchLink><br /><searchLink fieldCode="DE" term="%22X-ray+binaries%22">X-ray binaries</searchLink><br /><searchLink fieldCode="DE" term="%22Astronomy%22">Astronomy</searchLink><br /><searchLink fieldCode="DE" term="%22Computer+simulation%22">Computer simulation</searchLink><br /><searchLink fieldCode="DE" term="%22Space+plasmas%22">Space plasmas</searchLink>
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  Data: We present the first three-dimensional simulations of the evolution of a microquasar jet inside the binary star system. The aim is to study the interaction of these jets with the stellar wind from a massive companion and the possible locations of high-energy emission sites. We have simulated two jets with different injection power in order to give a hint on the minimum power required for the jet to escape the system and become visible in larger scales. In the setup, we include a massive star wind filling the grid through which the jet evolves. We show that jets should have powers of the order of 1037 erg s-1 or more in order not to be destroyed by the stellar wind. The jet–wind interaction results in regions in which high-energy emission could be produced. These results imply the possible existence of a population of X–ray binaries undetected in the radio band due to jet disruption inside the region dominated by the stellar wind. [ABSTRACT FROM AUTHOR]
– Name: AbstractSuppliedCopyright
  Label:
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  Data: <i>Copyright of International Journal of Modern Physics D: Gravitation, Astrophysics & Cosmology is the property of World Scientific Publishing Company and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.)
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        Value: 10.1142/S0218271810017032
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      – Code: eng
        Text: English
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        PageCount: 6
        StartPage: 791
    Subjects:
      – SubjectFull: Stellar winds
        Type: general
      – SubjectFull: X-ray binaries
        Type: general
      – SubjectFull: Astronomy
        Type: general
      – SubjectFull: Computer simulation
        Type: general
      – SubjectFull: Space plasmas
        Type: general
    Titles:
      – TitleFull: ON THE INTERACTION OF JETS WITH STELLAR WINDS IN MASSIVE X–RAY BINARIES.
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            NameFull: PERUCHO, MANEL
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            NameFull: BOSCH-RAMON, VALENTÍ
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            NameFull: KHANGULYAN, DMITRY
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            – D: 01
              M: 06
              Text: Jun2010
              Type: published
              Y: 2010
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            – TitleFull: International Journal of Modern Physics D: Gravitation, Astrophysics & Cosmology
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