Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....88..311h&link_type=abstract
Astronomy and Astrophysics, vol. 88, no. 3, Aug. 1980, p. 311-316.
Astronomy and Astrophysics
Astronomy
13
Galactic Nuclei, Quasars, Radio Emission, Spectral Line Width, Stellar Luminosity, Balmer Series, Correlation, Infrared Astronomy, Line Spectra
Scientific paper
Using recently published infrared and optical continuum fluxes and emission line parameters, the luminosity dependence of the properties of the broad-line region (BLR) in active nuclei and quasars were explored and an attempt was made to find systematic differences between optical and radio-selected BLR's in terms of these luminosity dependences. It is found that most properties of the BLR are not strongly luminosity dependent, with the He II 4686 A/H-beta and Fe II/H-beta line ratios being two exceptions. Interpretation in terms of a 'softening' of the ionizing continuum with increasing luminosity is discussed. It is found that BLR's occurring in conjunction with extended and strong radio emission are peculiar in many ways. When such BLR's are in radio galaxies, they often have abnormally large H-alpha/H-beta, forbidden O III/H-alpha, weak He II 4686, and weak He I 5876. Along with quasars of the same radio class, they have weak Fe II emission and abnormally broad Balmer lines.
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