How does a secular instability grow in a hyperaccretion flow?

Hyperaccretion flows with mass accretion rates far above the Eddington rate have an N-shaped equilibrium curve on the Σ– $\skew{3}\dot{M}$ plane (with Σ and $\skew{3}\dot{M}$ being surface density and mass accretion rate, respectively). The accretion flow on the lower Σ branch of the N-shape is opti...

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Veröffentlicht in:	Publications of the Astronomical Society of Japan 2015-10, Vol.67 (5)
Hauptverfasser:	Kimura, Mariko, Mineshige, Shin, Kawanaka, Norita
Format:	Artikel
Sprache:	eng
Online-Zugang:	Volltext
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