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• W2980772444 abstract "Blue-shifted Broad Absorption Lines (BALs) detected in quasar's spectra are indicative of AGN outflows. We show, using 2D hydrodynamical simulations, that disruption of interstellar clouds by a fast AGN wind can lead to formation of cold, dense high speed blobs that give rise to broad absorption features in the transmission spectrum of the AGN continuum source. For a wind velocity of $0.1 c$ and sufficiently high cloud density ($n_{c}$ < $10^4$ cm$^{-3}$, depending on size), absorption troughs with velocities up to about $3000$ km s$^{-1}$ can be produced. For slower winds and/or lower cloud density the anticipated velocity of the absorbing clouds should be smaller." @default.
• W2980772444 created "2019-10-25" @default.
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• W2980772444 date "2019-12-09" @default.
• W2980772444 modified "2023-10-16" @default.
• W2980772444 title "BALQSO spectra explained by shock disruption of galactic clouds" @default.
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• W2980772444 doi "https://doi.org/10.1093/mnras/stz3352" @default.
• W2980772444 hasPublicationYear "2019" @default.
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