A search for radio spectral lines from SS433

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Hydrogen Clouds, Line Spectra, Radio Spectra, Stellar Mass Ejection, Hydrogen Recombinations, Radiative Recombination, Spectrum Analysis

Scientific paper

A search has been made for radio spectral lines associated with SS433, from 1345 to 1412.5 MHz. No evidence for lines with velocity widths from 9 to 7000 km/s was found to a best limit of 40 mJy. This lack of lines may be explained by a variety of line broadening or suppression mechanisms. Alternatively, radio line forming neutral or ionized hydrogen may be too tenuous to detect.

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