Spectroscopy of the QSO pair Q0028+003/Q0029+003

Details Spectroscopy of the QSO pair Q0028+003/Q0029+003 Spectroscopy of the QSO pair Q0028+003/Q0029+003

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...261l...7s&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 261, Oct. 1, 1982, p. L7-L12. Research supported by the Science and

Astronomy and Astrophysics

Astrophysics

36

Absorption Spectra, Astronomical Spectroscopy, Galactic Clusters, Line Spectra, Quasars, Red Shift, Calcium, Galactic Nuclei, Magnesium, Spectral Energy Distribution, Spectral Line Width

Scientific paper

It is hypothesized that a prominent, narrow absorption line system discovered in the spectrum of Q0029+003, at a redshift of 1.7334, and only 190 km/sec from the emission line redshift of Q0028+003, may be due to a galaxy located in a cluster containing the latter QSO. Alternatively, the absorption line system may arise in a halo associated with Q0028+003 and extending at least 520 kpc, which is the projected separation of the two QSOs at this redshift.

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