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- W2020379964 abstract "The strong absorption lines in the spectrum of the quasar Q0248 + 4302 are discussed. The absorption has been shown to be produced in a sinuous tidal tail which emanates from the nearby galaxy pair G0248 + 4302A,B. There is a velocity difference of about 260 km/s between the systemic redshift of the interacting galaxies and the redshift of the tidal tail at a galactocentric distance of about 11/h kpc. The large velocity spread observed in the tail gas is probably responsible for the unusual strength of the interstellar lines. 18 refs." @default.
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- W2020379964 date "1990-08-01" @default.
- W2020379964 modified "2023-09-27" @default.
- W2020379964 title "Absorption lines in the spectrum of Q0248 + 4302 due to a foreground tidal tail" @default.
- W2020379964 doi "https://doi.org/10.1086/185790" @default.
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