QSO Q1232 + 134 and the multiple redshifts

Details QSO Q1232 + 134 and the multiple redshifts QSO Q1232 + 134 and the multiple redshifts

Jan 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987sssmp..30...67h&link_type=abstract

Scientia Sinica, Series A - Mathematical, Physical, Astronomical and Technical Sciences (ISSN 0253-5831), vol. 30, Jan. 1987, p.

Astronomy and Astrophysics

Astronomy

Absorption Spectra, Emission Spectra, Line Spectra, Quasars, Red Shift, Astronomical Spectroscopy, Galactic Clusters

Scientific paper

Q1232 + 134 is a quasar that was discovered in the region of the Virgo cluster of galaxies in 1982. The results of the UK Schmidt objective-prism survey and spectroscopic observations using the Palomar 5-m telescope are introduced in this paper. All of the emission lines are listed; the corresponding redshift is Z(e) = 2.364 + or - 0.002. There are 29 absorption lines in the spectrum. Two absorption line redshift systems and a possible system have been found.

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