TL;DR
This paper revisits Newtonian spherically symmetric transonic accretion by incorporating the accreting matter's mass and introduces an iterative method, revealing changes in flow properties and phase portraits.
Contribution
It presents a novel iterative approach to include fluid mass effects in accretion flow analysis, altering critical flow characteristics.
Findings
Inclusion of fluid mass modifies critical points.
Flow topologies are significantly affected.
New iterative method improves modeling accuracy.
Abstract
Newtonian spherically symmetric transonic accretion has been studied by including the mass of the accreting matter, while considering the growth of the accretor itself to be negligibly small. A novel iterative method has been introduced to accomplish that task. It has been demonstrated that the inclusion of the mass of the fluid changes the critical properties of the flow as well as the topological phase portraits of the stationary integral solution.
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