A&A 370, 555-556 (2001)
DOI: 10.1051/0004-6361:20010425

Erratum: Circumstellar dust shells around long-period variables

IX. Molecular layers resulting from shocked carbon-rich atmospheres

Ch. Helling1 - J. M. Winters1,2,3

1 - Institut für Astronomie und Astrophysik, TU Berlin, Sekr. PN 8-1, Hardenbergstraße 36, 10623 Berlin, Germany
2 - Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
3 - DEMIRM, UMR8540, Observatoire de Paris, 61 Av. de l'Observatoire, 75014 Paris, France

A&A, 366, 229-240 (2001), DOI: 10.1051/0004-6361:20000206

By mistake, Fig. 3 has been plotted again in Fig. 4 (p. 233). The correct figures are given below.

  \begin{figure*}\hbox{\epsfig{file=Fig1Erratumh2137.eps, width=9cm, height=11cm}\epsfig{file=Fig2Erratumh2137.eps, width=9cm, height=11cm} }
\end{figure*} Figure 1: Molecular number densities n for Model F (small constant gas opacity) in the hydrostatic case (l.h.s.) and for the hydrodynamic case (r.h.s.). The instant of time depicted is the same as in Fig. 1. (Upper panel: temperature (dashed black-static, full black-dynamic), gas density (dashed grey-static, full grey-dynamic))
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  \begin{figure*}\hbox{\epsfig{file=Fig3Erratum2137.eps, width=9cm, height=11cm}\epsfig{file=Fig4Erratum2137.eps, width=9cm, height=11cm} }
\end{figure*} Figure 2: Same as Fig. 3 for Model B (Plank mean gas opacity). The instant of time depicted is the same as in Fig. 2
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Copyright ESO 2001