Structure and Magnetic Fields in the Precessing Jet System SS 433 II. Intrinsic Brightness of the Je...
Structure and Magnetic Fields in the Precessing Jet System SS 433 II. Intrinsic Brightness of the Jets
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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Contents
Deep Very Large Array imaging of the binary X-ray source SS 433, sometimes classified as a microquasar, has been used to study the intrinsic brightness distribution and evolution of its radio jets. The intrinsic brightness of the jets as a function of age at emission of the jet material tau is recovered by removal of the Doppler boosting and projec...
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Full title
Structure and Magnetic Fields in the Precessing Jet System SS 433 II. Intrinsic Brightness of the Jets
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TN_cdi_proquest_journals_2082500549
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2082500549
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E-ISSN
2331-8422
DOI
10.48550/arxiv.1003.0145
