Possible origin of the radio emission from SS433 jets
| العنوان: | Possible origin of the radio emission from SS433 jets |
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| المؤلفون: | P. N. Okeke, M. W. Anyakoha, S. S. Nweze |
| المصدر: | Astrophysics and Space Science. 173:257-263 |
| بيانات النشر: | Springer Science and Business Media LLC, 1990. |
| سنة النشر: | 1990 |
| مصطلحات موضوعية: | Physics, Jet (fluid), Radio galaxy, Astrophysics::High Energy Astrophysical Phenomena, X-ray binary, Inelastic collision, Flux, Astronomy and Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, Space and Planetary Science, Thermal, High Energy Physics::Experiment, Emission spectrum, Atomic number |
| الوصف: | It is shown that radio emission from the jet of the galactic source SS433 as well as the variability of its flux density could be accounted for by the inelastic collision model. Variability in the jet flux is attributed mainly to the variability in the thermal proton number density available in the jet regions. |
| تدمد: | 1572-946X 0004-640X |
| URL الوصول: | https://explore.openaire.eu/search/publication?articleId=doi_________::48275bfce952b9f37a91fe9d1186d259 https://doi.org/10.1007/bf00643935 |
| حقوق: | CLOSED |
| رقم الأكسشن: | edsair.doi...........48275bfce952b9f37a91fe9d1186d259 |
| قاعدة البيانات: | OpenAIRE |
Find this article in full text from Springer Verlag. | تدمد: | 1572946X 0004640X |
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