Erratum: ``Balmer Lines as Diagnostics of Physical Conditions in Active Galactic Nuclei Broad Emission Line Regions'' (ApJ, 599, 140 [2003])

Details Erratum: ``Balmer Lines as Diagnostics of Physical Conditions in Active Galactic Nuclei Broad Emission Line Regions'' (ApJ, 599, 140 [2003]) Erratum: ``Balmer Lines as Diagnostics of Physical Conditions in Active Galactic Nuclei Broad Emission Line Regions'' (ApJ, 599, 140 [2003])

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006apj...650.1217p&link_type=abstract

The Astrophysical Journal, Volume 650, Issue 2, pp. 1217-1218.

Astronomy and Astrophysics

Astrophysics

12

Scientific paper

In our original paper, an error was made in the application of equation (2),log(In)=log(Iul×λ)/(guAul)=B-AEu (2)here the temperature parameter should have the value A=log(e)/(kT)~0.4323/(kT). Consequently, the temperature obtained in the paper should be rescaled as T'e=Te×log(e)~0.4343×Te, where Te denotes the temperatures given in the paper. The corrected Figures 5 and 7 are given below. This error does not affect our general conclusions; only the estimated BLR electron temperatures where PLTE exist are smaller than noted in the paper.

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