Formation of Quasar Clouds by Thermal Instability in the Presence of Alfven Wave Heating: Erratum

Details Formation of Quasar Clouds by Thermal Instability in the Presence of Alfven Wave Heating: Erratum Formation of Quasar Clouds by Thermal Instability in the Presence of Alfven Wave Heating: Erratum

Aug 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994apj...431..450g&link_type=abstract

Astrophysical Journal v.431, p.450

Astronomy and Astrophysics

Astronomy

Errata, Addenda

Scientific paper

In the paper "Formation of Quasar Clouds by Thermal Instability in the Presence of Alfven Wave Heating" by D. R. Goncalves, V. Jatenco-Pereira, and R. Opher (ApJ, 414,57 [1993]), the calculations of Figures 2-4 have been performed with greater accuracy. The basic conclusions of the paper are unaltered (although the figures are changed somewhat), since the stable two-phase equilibrium exists until log P <= -3, log P <= -3.32, and log P~ -2 in Figures 2,3, and 4, respectively. The differences in the figures appear at low pressures. The stable two-phase equilibrium begins at lower pressures in the revised figures. The new result for the broad line region of quasars implies the existence of thermal instability at lower pressures.

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