Spectroscopy of the fuzz associated with four quasars

Details Spectroscopy of the fuzz associated with four quasars Spectroscopy of the fuzz associated with four quasars

Feb 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...265l...1b&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 265, Feb. 1, 1983, p. L1-L5.

Astronomy and Astrophysics

Astrophysics

31

Astronomical Spectroscopy, Galactic Nuclei, Quasars, Red Shift, Hydrogen Clouds, Luminosity, Spectrum Analysis

Scientific paper

The spectral features detected in the fuzz of four probable quasars spanning the z range of 0.036-0.37 are reported; the objects studied are 0351 + 026 (z = 0.036), 1059 + 730 (z = 0.089), 0845 + 378 (z = 0.307), and 3C 48 (z = 0.368). The results indicate that apparently some (and probably all) low-redshift quasars are embedded in fuzz whose size, morphology, absolute magnitude, and spectroscopic character are those of a galaxy. Thus, it appears virtually certain that quasars are the active nuclei of galaxies.

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