next previous
Up: Stellar parameters for Pop II atmospheres


Online material


  \begin{figure}\par\resizebox{9cm}{!}
{\includegraphics[0.5,0.][500,700]{ms1683fA1.ps}}\end{figure} Figure A.1: Comparison of IUE low-resolution spectra (dashed line) of BD+32 2188 and HD 128801 with energy distributions computed with parameters: (1) from KCC (panel OLD, thin line); (2) from the fit of the IUE spectra to the old-ODF grids (panel OLD, thick line); (3) from the fit of the IUE spectra to the new-ODF grids (panel NEW, thick line). The flux units are erg sec-1 cm-2 Å-1. See text of Appendix A for more details.


  \begin{figure}\par\resizebox{9cm}{!}
{\includegraphics[0.5,0.][500,700]{ms1683fA2.ps}}\end{figure} Figure A.2: The same as Fig. A.1, but for BD+00 145 and HD 87112.


  \begin{figure}
\par\resizebox{9cm}{!}
{\includegraphics[20,5][477,694]{ms1683fA3.ps}}\end{figure} Figure A.3: The same as Fig. A.1, but for HD 106304 and HD 117880.


  \begin{figure}\par\resizebox{9cm}{!}
{\includegraphics[0.5,0.][500,700]{ms1683fA4.ps}}\end{figure} Figure A.4: The same as Fig. A.1, but for HD 213468 and HD 130095.


  \begin{figure}\par\resizebox{9cm}{!}
{\includegraphics[0.5,0.][500,730]{ms1683fA5.ps}}
\par\end{figure} Figure A.5: The same as Fig. A.1, but for HD 167105 and HD 14829.


  \begin{figure}\par\resizebox{9cm}{!}
{\includegraphics[0.5,0.][500,730]{ms1683fA6.ps}}\end{figure} Figure A.6: The same as Fig. A.1, but for HD 130201 and HD 74721.


  \begin{figure}\par\resizebox{9cm}{!}
{\includegraphics[0.5,0.][500,650]{ms1683fA7.ps}}\end{figure} Figure A.7: The same as Fig. A.1, but for BD+42 2309 and HD 78913.


  \begin{figure}\par\resizebox{9cm}{!}
{\includegraphics[0.5,0.][500,730]{ms1683fA8.ps}}\end{figure} Figure A.8: The same as Fig. A.1, but for HD 139961 and HD 109995.


  \begin{figure}\par\resizebox{9cm}{!}
{\includegraphics[0.5,0.][500,670]{ms1683fA9.ps}}\end{figure} Figure A.9: The same as Fig. A.1, but for HD 4850 and HD 93329.


  \begin{figure}\par\resizebox{9cm}{!}
{\includegraphics[0.5,0.][500,670]{ms1683fA10.ps}}\end{figure} Figure A.10: The same as Fig. A.1, but for HD 60778 and HD 86986.


  \begin{figure}\par\resizebox{9cm}{!}
{\includegraphics[0.5,0.][500,700]{ms1683fA11.ps}}\end{figure} Figure A.11: The same as Fig. A.1, but for HD 8376 and HD 13780.


  \begin{figure}\par\resizebox{9cm}{!}
{\includegraphics[0.5,0.][500,750]{ms1683fA12.ps}}\end{figure} Figure A.12: The same as Fig. A.1, but for HD 87047 and HD 31943.


  \begin{figure}\par\resizebox{9cm}{!}
{\includegraphics[0.5,0.][500,720]{ms1683fA13.ps}}\end{figure} Figure A.13: The same as Fig. A.1, but for HD 180903 and HD 252940.


  \begin{figure}\par\resizebox{9cm}{!}
{\includegraphics[0.5,0.][500,720]{ms1683fA14.ps}}\end{figure} Figure A.14: The same as Fig. A.1, but for HD 2857 and HD 161817.


  \begin{figure}\par\resizebox{9cm}{!}
{\includegraphics[0.5,0.][500,450]{ms1683fA15.ps}}\end{figure} Figure A.15: The same as Fig. A.1, but for HD 202759.


next previous
Up: Stellar parameters for Pop II atmospheres

Copyright ESO 2001