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- W2023166210 startingPage "1844" @default.
- W2023166210 abstract "The chance projection of the disk of Mrk 1456 onto a background QSO is similar to the case of SBS 1543+593-HS 1543+5921. Mrk 1456 is a luminous, late-type spiral galaxy at z ? 0.05. Although the QSO, SDSS J114719.90+522923.2 at z ? 2, has not yet been observed with ultraviolet spectroscopy, it shows strong Ca II absorption at the redshift of Mrk 1456, which gives evidence that it is a possible damped Ly? absorber. Spectroscopy of the star-forming nucleus of Mrk 1456 allows us to apply emission-line diagnostics to infer the chemical abundances at the center of the galaxy and to make a prediction of the expected metallicity on the sight line to the QSO." @default.
- W2023166210 created "2016-06-24" @default.
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- W2023166210 date "2006-09-22" @default.
- W2023166210 modified "2023-09-27" @default.
- W2023166210 title "Galaxies in Front of Quasars: Markarian 1456 and SDSS J114719.90+522923.2" @default.
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- W2023166210 doi "https://doi.org/10.1086/507789" @default.
- W2023166210 hasPublicationYear "2006" @default.
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