SS433's circumbinary ring and accretion disc viewed through its attenuating disc wind

We present optical spectroscopy of the microquasar SS433 covering a significant fraction of a precessional cycle of its jet axis. The components of the prominent stationary H-alpha and H-beta lines are mainly identified as arising from three emitting regions: (i) a super-Eddington accretion disc win...

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Bibliografski detalji
Glavni autori: Perez, S, Blundell, K
Format: Journal article
Jezik:English
Izdano: 2010

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