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- W2050871082 abstract "It is suggested that the salient features of the velocity structure underlying the broad absorption lines of some quasars (BAL QSOs) are produced in a time-variable, freely expanding wind. The observed span in velocities of absorbing elements is produced by time variations in the ejection speed of the gas and not by acceleration of the gas in the absorption region, as must be the case in steady state models. Such a wind is characterized by time-dependent mass injection and energy injection rates. 12 refs." @default.
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- W2050871082 date "1990-02-01" @default.
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- W2050871082 title "A variable flow as the underpinning of broad absorption lines in quasi-stellar objects" @default.
- W2050871082 doi "https://doi.org/10.1086/185645" @default.
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