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Here we propose a more direct test of the observed correlation between mass accretion and ejection by using UV emission to detect accreting gas and centimeter emission to trace the jet while disentangling the influence of high-energy X-ray radiation from the star.
A brief epoch of rapid mass transfer is expected to occur in most accreting binary systems, and can readily exceed the Eddington mass accretion rate by up to several orders of magnitude.
The mass accretion rate (solar mass per year).
To what extent do outflows regulate the protostellar mass accretion process?
The mass accretion rate in units of 10^18 g/s.
Hosokawa, T., Yorke, H. W., Inayoshi, K., Omukai, K. & Yoshida, N. Formation of primordial supermassive stars by rapid mass accretion.
Donati, J.-F. et al. The close classical T Tauri binary V4046 Sgr: complex magnetic fields and distributed mass accretion.
Love, S. G. & Brownlee, D. E. A direct measurement of the terrestrial mass accretion rate of cosmic dust.
I shall present and discuss the evidence for high mass accretion rate disks in two recent novae.
Energetic outflows appear to occur in conjunction with active mass accretion onto supermassive black holes.
This expression also holds when mass accretion is thwarted, e.g. by a wind, as long as the wind-cloud interaction is sufficiently confined spatially.
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CEO of Professional Science Editing for Scientists @ prosciediting.com