Observations of the Einstein Cross 2237+030 with the TIGER Integral Field Spectrograph

Details Observations of the Einstein Cross 2237+030 with the TIGER Integral Field Spectrograph Observations of the Einstein Cross 2237+030 with the TIGER Integral Field Spectrograph

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...208l..15a&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 208, no. 1-2, Jan. 1989, p. L15-L18.

Astronomy and Astrophysics

Astrophysics

21

Galactic Nuclei, Gravitational Lenses, Line Spectra, Quasars, Spectrographs, Image Resolution, Imaging Spectrometers, Spectrum Analysis, Star Clusters

Scientific paper

Observations of the Einstein Cross 2237+030 with the TIGER Integral
Field Spectrograph (IFS) strongly confirm the gravitational lens
hypothesis. C III semiforbidden emission-line and Mg I absorption-line
mappings are used to discriminate the quasar images and the galactic
nucleus.

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