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On Compact Steep Spectrum Sources and Jet Production

Received: 22 January 2015     Accepted: 6 February 2015     Published: 16 February 2015
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Abstract

In this work, we show the possibility that jet production by magnetization predominates over other mechanisms of jet production in radio sources with low power output. We obtain estimates of accretion induced magnetic field and jet-driving magnetic field of compact steep spectrum sources in our sample using analytical methods.A possible implication of the results obtained through simple linear regression analyses of the data estimated for the two aforementioned fields is that jet production by magnetization predominates in the CSS radio sources with lower power output; while in those with higher power output, the converse may be the case – some other processes,such as; hydrodynamic, thermal, and radiation pressures may predominate over jet magnetization.

Published in American Journal of Astronomy and Astrophysics (Volume 3, Issue 1)
DOI 10.11648/j.ajaa.20150301.11
Page(s) 1-5
Creative Commons

This is an Open Access article, distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution and reproduction in any medium or format, provided the original work is properly cited.

Copyright

Copyright © The Author(s), 2015. Published by Science Publishing Group

Keywords

Jet, Accretion, Magnetization, Steep Spectrum, Radio Sources

References
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  • APA Style

    Ezeugo Jeremiah Chukwuemerie. (2015). On Compact Steep Spectrum Sources and Jet Production. American Journal of Astronomy and Astrophysics, 3(1), 1-5. https://doi.org/10.11648/j.ajaa.20150301.11

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    ACS Style

    Ezeugo Jeremiah Chukwuemerie. On Compact Steep Spectrum Sources and Jet Production. Am. J. Astron. Astrophys. 2015, 3(1), 1-5. doi: 10.11648/j.ajaa.20150301.11

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    AMA Style

    Ezeugo Jeremiah Chukwuemerie. On Compact Steep Spectrum Sources and Jet Production. Am J Astron Astrophys. 2015;3(1):1-5. doi: 10.11648/j.ajaa.20150301.11

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  • @article{10.11648/j.ajaa.20150301.11,
      author = {Ezeugo Jeremiah Chukwuemerie},
      title = {On Compact Steep Spectrum Sources and Jet Production},
      journal = {American Journal of Astronomy and Astrophysics},
      volume = {3},
      number = {1},
      pages = {1-5},
      doi = {10.11648/j.ajaa.20150301.11},
      url = {https://doi.org/10.11648/j.ajaa.20150301.11},
      eprint = {https://article.sciencepublishinggroup.com/pdf/10.11648.j.ajaa.20150301.11},
      abstract = {In this work, we show the possibility that jet production by magnetization predominates over other mechanisms of jet production in radio sources with low power output. We obtain estimates of accretion induced magnetic field and jet-driving magnetic field of compact steep spectrum sources in our sample using analytical methods.A possible implication of the results obtained through simple linear regression analyses of the data estimated for the two aforementioned fields is that jet production by magnetization predominates in the CSS radio sources with lower power output; while in those with higher power output, the converse may be the case – some other processes,such as; hydrodynamic, thermal, and radiation pressures may predominate over jet magnetization.},
     year = {2015}
    }
    

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    T1  - On Compact Steep Spectrum Sources and Jet Production
    AU  - Ezeugo Jeremiah Chukwuemerie
    Y1  - 2015/02/16
    PY  - 2015
    N1  - https://doi.org/10.11648/j.ajaa.20150301.11
    DO  - 10.11648/j.ajaa.20150301.11
    T2  - American Journal of Astronomy and Astrophysics
    JF  - American Journal of Astronomy and Astrophysics
    JO  - American Journal of Astronomy and Astrophysics
    SP  - 1
    EP  - 5
    PB  - Science Publishing Group
    SN  - 2376-4686
    UR  - https://doi.org/10.11648/j.ajaa.20150301.11
    AB  - In this work, we show the possibility that jet production by magnetization predominates over other mechanisms of jet production in radio sources with low power output. We obtain estimates of accretion induced magnetic field and jet-driving magnetic field of compact steep spectrum sources in our sample using analytical methods.A possible implication of the results obtained through simple linear regression analyses of the data estimated for the two aforementioned fields is that jet production by magnetization predominates in the CSS radio sources with lower power output; while in those with higher power output, the converse may be the case – some other processes,such as; hydrodynamic, thermal, and radiation pressures may predominate over jet magnetization.
    VL  - 3
    IS  - 1
    ER  - 

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Author Information
  • Department of Physics and Industrial physics, NnamdiAzikiwe University, Awka, Anambra State, Nigeria

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