An absorption line study of galaxies at high redshift

Details An absorption line study of galaxies at high redshift An absorption line study of galaxies at high redshift

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.118..501m&link_type=abstract

(IAU, Asian-Pacific Regional Meeting, 3rd, Kyoto, Japan, Sept. 30-Oct. 5, 1984) Astrophysics and Space Science (ISSN 0004-640X),

Astronomy and Astrophysics

Astrophysics

3

Absorption Spectra, Galactic Structure, Line Spectra, Red Shift, Spectrum Analysis, Abundance, Spectral Resolution, Velocity Distribution

Scientific paper

Complex velocity structure is revealed in several absorption systems in
the spectrum of 0215+015 (z = 1.715) at resolutions of 20 - 30 km
s-1 FWHM. Striking differences are found in the relative
strengths of low to high ions among the components, reinforcing the
interpretation of these systems as intervening galaxies.

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