The physical parameters of the microquasar S26 in the Sculptor Group galaxy NGC 7793
NGC 7793-S26 is an extended source (350pc × 185pc) previously studied in the radio, optical and X-ray domains. It has been identified as a microquasar which has inflated a superbubble. We used integral-field spectra from the Wide-Field Spectrograph on th
|Collections||ANU Research Publications|
|Source:||Monthly Notices of the Royal Astronomical Society|
|01_Dopita_The_physical_parameters_of_the_2012.pdf||664.61 kB||Adobe PDF|
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