GAMMA-RAYS FROM SS 433 AND ITS INTERACTION WITH THE W50 NEBULA.

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Title: GAMMA-RAYS FROM SS 433 AND ITS INTERACTION WITH THE W50 NEBULA.
Authors: BORDAS, POL1 pbordas@am.ub.es, BOSCH-RAMON, VALENTÍ2 vbosch@mpi-hd.mpg.de, PAREDES, JOSEP MARIA1 jmparedes@ub.edu
Source: International Journal of Modern Physics D: Gravitation, Astrophysics & Cosmology. Jun2010, Vol. 19 Issue 6, p749-755. 7p. 1 Diagram, 2 Charts, 2 Graphs.
Subjects: Gamma rays, Nebulae, Atomization, Properties of matter, Galaxies
Abstract: We investigate the production of gamma-rays in the inner regions of SS 433 and in its interaction between its jets and the W50 nebula. We estimate the VHE emission that can be generated within the jets at distances ≳ 1013 cm from the compact object. We also apply a theoretical model of the jet/medium interaction to SS 433/W50. We compare the predicted fluxes to observations of SS 433 at TeV energies, and derive new constraints of the physical properties of this system. [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.)
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  Data: GAMMA-RAYS FROM SS 433 AND ITS INTERACTION WITH THE W50 NEBULA.
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  Data: <searchLink fieldCode="DE" term="%22Gamma+rays%22">Gamma rays</searchLink><br /><searchLink fieldCode="DE" term="%22Nebulae%22">Nebulae</searchLink><br /><searchLink fieldCode="DE" term="%22Atomization%22">Atomization</searchLink><br /><searchLink fieldCode="DE" term="%22Properties+of+matter%22">Properties of matter</searchLink><br /><searchLink fieldCode="DE" term="%22Galaxies%22">Galaxies</searchLink>
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  Data: We investigate the production of gamma-rays in the inner regions of SS 433 and in its interaction between its jets and the W50 nebula. We estimate the VHE emission that can be generated within the jets at distances ≳ 1013 cm from the compact object. We also apply a theoretical model of the jet/medium interaction to SS 433/W50. We compare the predicted fluxes to observations of SS 433 at TeV energies, and derive new constraints of the physical properties of this system. [ABSTRACT FROM AUTHOR]
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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/S0218271810016646
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        Type: general
      – SubjectFull: Nebulae
        Type: general
      – SubjectFull: Atomization
        Type: general
      – SubjectFull: Properties of matter
        Type: general
      – SubjectFull: Galaxies
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      – TitleFull: GAMMA-RAYS FROM SS 433 AND ITS INTERACTION WITH THE W50 NEBULA.
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              Text: Jun2010
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