SS 433: O I lines and the circumbinary disk
M G Bowler
TL;DR
This paper investigates atomic oxygen emission lines at 8446 Angstroms in SS 433, revealing a stable circumbinary disk unaffected by optical outbursts and radio flares.
Contribution
It provides evidence of a persistent circumbinary disk in SS 433 using O I emission lines, highlighting its stability during energetic events.
Findings
O I 8446 Angstroms trace the circumbinary disk
The disk remains undisturbed during outbursts
Stable emission indicates a persistent structure
Abstract
Atomic oxygen emission at 8446 Angstroms traces the stable circumbinary disk undisturbed through an optical outburst and accompanying radio flare
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Stellar, planetary, and galactic studies · Galaxies: Formation, Evolution, Phenomena