@article {Ray:September 2003:0035-8711:83,
	author = "Ray A.K.",
	title = "Linearized perturbation on stationary inflow solutions in an inviscid and thin accretion disc",
	journal = "Monthly Notices of the Royal Astronomical Society",
	volume = "344",
	year = "September 2003",
	abstract = "<P></P>The influence of a linearized perturbation on stationary inflow solutions in an inviscid and thin accretion disc has been studied here, and it has been argued that a perturbative technique would indicate that all possible classes of inflow solutions would be stable. The choice of the driving potential, Newtonian or pseudo-Newtonian, would not particularly affect the arguments which establish the stability of solutions. It has then been surmised that in the matter of the selection of a particular solution, adoption of a non-perturbative technique, based on a more physical criterion, as in the case of the selection of the transonic solution in spherically symmetric accretion, would give a more conclusive indication concerning the choice of a particular branch of the flow.",
	pages = "83-88(6)",
	url = "http://www.ingentaconnect.com/content/bsc/mnr/2003/00000344/00000001/art00011"
	doi = "doi:10.1046/j.1365-8711.2003.06796.x"
}