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Astron. Astrophys. 323, 286 (1997)

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Line-blanketed model atmospheres for R Coronae Borealis stars and hydrogen-deficient carbon stars

Martin Asplund 1, Bengt Gustafsson 1, Dan Kiselman 2, 3 and Kjell Eriksson 1

1 Astronomiska observatoriet, Box 515, S-751 20 Uppsala, Sweden
2 NORDITA, Blegdamsvej 17, DK-2100 Copenhagen O, Denmark
3 present address: Stockholms observatorium, S-133 36 Saltsjöbaden, Sweden

Astron. Astrophys. 318, 521-534


Unfortunately the gravities of the models displayed in Fig. 6 and the tickmarks for the optical depths for the comparison model of Schönberner have been mislabeled. The correct figure and caption are shown below. The temperature difference between the two models amounts to about 700 K at the surface (