Analysis of hydrogen-rich magnetic white dwarfs detected in the Sloan Digital Sky Survey

B. Külebi; S. Jordan; F. Euchner; B. T. Gänsicke; H. Hirsch

doi:10.1051/0004-6361/200912570

Free Access

Issue		A&A Volume 506, Number 3, November II 2009


Page(s)		1341 - 1350
Section		Stellar atmospheres
DOI		https://doi.org/10.1051/0004-6361/200912570
Published online		27 August 2009

Online Material

Table 3: Model fits with centered dipole and offset dipole models with comparison to literature values. The columns indicate the SDSS name of the object; the plate, Modified Julian Date and fiber ids of the observations; the dipole magnetic field strength of the centered dipole, the inclination with respect to the line of sight of the centered dipole, the dipole magnetic field strength of the offset dipole, the inclination with respect to the line of sight of the offset dipole, the offset along the axis of the magnetic field in terms of the stellar radius, and finally comments indicate the model parameters from the literature (i.e. Vanlandingham et al. 2005; Schmidt et al. 2003; Gänsicke et al. 2002)

Appendix A: Figures of all fits not shown in the printed version

$\begin{figure}\par\resizebox{!}{17cm}{\includegraphics[viewport=45 39 595 812]{12570f09.eps}} \end{figure}$	Figure A.1: Color version of Fig. 1.
Open with DEXTER

$\begin{figure}\par\resizebox{!}{17cm}{\includegraphics[viewport=45 39 595 812]{12570f10.eps}} \end{figure}$	Figure A.2: Color version of Fig. 2.
Open with DEXTER

$\begin{figure}\par\resizebox{!}{17cm}{\includegraphics[viewport=45 39 595 812]{12570f11.eps}} \end{figure}$	Figure A.3: Fits of observed spectra of DAHs from the SDSS to centered magnetic dipoles with a polar field strength $B_{\rm p}$ ( left) and dipoles shifted by $z_{\rm off}$ stellar radii along the dipole axis ( right).
Open with DEXTER

$\begin{figure}\par\resizebox{!}{17cm}{\includegraphics[viewport=45 39 595 812]{12570f12.eps}} \end{figure}$	Figure A.4: Fits of observed spectra of DAHs from the SDSS to centered magnetic dipoles with a polar field strength $B_{\rm p}$ ( left) and dipoles shifted by $z_{\rm off}$ stellar radii along the dipole axis ( right).
Open with DEXTER

$\begin{figure}\par\resizebox{!}{17cm}{\includegraphics[viewport=45 39 595 812]{12570f13.eps}} \end{figure}$	Figure A.5: Fits of observed spectra of DAHs from the SDSS to centered magnetic dipoles with a polar field strength $B_{\rm p}$ ( left) and dipoles shifted by $z_{\rm off}$ stellar radii along the dipole axis ( right).
Open with DEXTER

$\begin{figure}\par\resizebox{!}{17cm}{\includegraphics[viewport=45 39 595 812]{12570f14.eps}} \end{figure}$	Figure A.6: Fits of observed spectra of DAHs from the SDSS to centered magnetic dipoles with a polar field strength $B_{\rm p}$ ( left) and dipoles shifted by $z_{\rm off}$ stellar radii along the dipole axis ( right).
Open with DEXTER

$\begin{figure}\par\resizebox{!}{17cm}{\includegraphics[viewport=45 39 595 812]{12570f15.eps}} \end{figure}$	Figure A.7: Fits of observed spectra of DAHs from the SDSS to centered magnetic dipoles with a polar field strength $B_{\rm p}$ ( left) and dipoles shifted by $z_{\rm off}$ stellar radii along the dipole axis ( right).
Open with DEXTER

$\begin{figure}\par\resizebox{!}{17cm}{\includegraphics[viewport=45 39 595 812]{12570f16.eps}} \end{figure}$	Figure A.8: Fits of observed spectra of DAHs from the SDSS to centered magnetic dipoles with a polar field strength $B_{\rm p}$ ( left) and dipoles shifted by $z_{\rm off}$ stellar radii along the dipole axis ( right).
Open with DEXTER

$\begin{figure}\par\resizebox{!}{17cm}{\includegraphics[viewport=45 39 595 812]{12570f17.eps}} \end{figure}$	Figure A.9: FFits of observed spectra of DAHs from the SDSS to centered magnetic dipoles with a polar field strength $B_{\rm p}$ ( left) and dipoles shifted by $z_{\rm off}$ stellar radii along the dipole axis ( right).
Open with DEXTER

$\begin{figure}\par\resizebox{!}{17cm}{\includegraphics[viewport=45 39 595 812]{12570f18.eps}} \end{figure}$	Figure A.10: Fits of observed spectra of DAHs from the SDSS to centered magnetic dipoles with a polar field strength $B_{\rm p}$ ( left) and dipoles shifted by $z_{\rm off}$ stellar radii along the dipole axis ( right).
Open with DEXTER

$\begin{figure}\par\resizebox{!}{17cm}{\includegraphics[viewport=45 39 595 812]{12570f19.eps}} \end{figure}$	Figure A.11: Fits of observed spectra of DAHs from the SDSS to centered magnetic dipoles with a polar field strength $B_{\rm p}$ ( left) and dipoles shifted by $z_{\rm off}$ stellar radii along the dipole axis ( right).
Open with DEXTER

$\begin{figure}\par\resizebox{!}{17cm}{\includegraphics[viewport=45 39 595 812]{12570f20.eps}} \end{figure}$	Figure A.12: Fits of observed spectra of DAHs from the SDSS to centered magnetic dipoles with a polar field strength $B_{\rm p}$ ( left) and dipoles shifted by $z_{\rm off}$ stellar radii along the dipole axis ( right).
Open with DEXTER

$\begin{figure}\par\resizebox{!}{17cm}{\includegraphics[viewport=45 39 595 812]{12570f21.eps}} \end{figure}$	Figure A.13: Fits of observed spectra of DAHs from the SDSS to centered magnetic dipoles with a polar field strength $B_{\rm p}$ ( left) and dipoles shifted by $z_{\rm off}$ stellar radii along the dipole axis ( right).
Open with DEXTER

$\begin{figure}\par\resizebox{!}{17cm}{\includegraphics[viewport=45 39 595 812]{12570f22.eps}} \end{figure}$	Figure A.14: Fits of observed spectra of DAHs from the SDSS to centered magnetic dipoles with a polar field strength $B_{\rm p}$ ( left) and dipoles shifted by $z_{\rm off}$ stellar radii along the dipole axis ( right).
Open with DEXTER

$\begin{figure}\par\resizebox{!}{17cm}{\includegraphics[viewport=45 39 595 812]{12570f23.eps}} \end{figure}$	Figure A.15: Fits of observed spectra of DAHs from the SDSS to centered magnetic dipoles with a polar field strength $B_{\rm p}$ ( left) and dipoles shifted by $z_{\rm off}$ stellar radii along the dipole axis ( right).
Open with DEXTER

$\begin{figure}\par\resizebox{!}{17cm}{\includegraphics[viewport=45 39 595 812]{12570f24.eps}} \end{figure}$	Figure A.16: Fits of observed spectra of DAHs from the SDSS to centered magnetic dipoles with a polar field strength $B_{\rm p}$ ( left) and dipoles shifted by $z_{\rm off}$ stellar radii along the dipole axis ( right).
Open with DEXTER

$\begin{figure}\par\resizebox{!}{17cm}{\includegraphics[viewport=45 39 595 812]{12570f25.eps}} \end{figure}$	Figure A.17: Fits of observed spectra of DAHs from the SDSS to centered magnetic dipoles with a polar field strength $B_{\rm p}$ ( left) and dipoles shifted by $z_{\rm off}$ stellar radii along the dipole axis ( right).
Open with DEXTER

$\begin{figure}\par\resizebox{!}{17cm}{\includegraphics[viewport=45 39 595 812]{12570f26.eps}} \end{figure}$	Figure A.18: Fits of observed spectra of DAHs from the SDSS to centered magnetic dipoles with a polar field strength $B_{\rm p}$ ( left) and dipoles shifted by $z_{\rm off}$ stellar radii along the dipole axis ( right).
Open with DEXTER

$\begin{figure}\par\resizebox{!}{17cm}{\includegraphics[viewport=45 39 595 812]{12570f27.eps}} \end{figure}$	Figure A.19: Fits of observed spectra of DAHs from the SDSS to centered magnetic dipoles with a polar field strength $B_{\rm p}$ ( left) and dipoles shifted by $z_{\rm off}$ stellar radii along the dipole axis ( right).
Open with DEXTER

$\begin{figure}\par\resizebox{!}{17cm}{\includegraphics[viewport=45 39 595 812]{12570f28.eps}} \end{figure}$	Figure A.20: Fits of observed spectra of DAHs from the SDSS to centered magnetic dipoles with a polar field strength $B_{\rm p}$ ( left) and dipoles shifted by $z_{\rm off}$ stellar radii along the dipole axis ( right).
Open with DEXTER

$\begin{figure}\par\resizebox{!}{17cm}{\includegraphics[viewport=45 39 595 812]{12570f29.eps}} \end{figure}$	Figure A.21: Fits of observed spectra of DAHs from the SDSS to centered magnetic dipoles with a polar field strength $B_{\rm p}$ ( left) and dipoles shifted by $z_{\rm off}$ stellar radii along the dipole axis ( right).
Open with DEXTER

$\begin{figure}\par\resizebox{!}{17cm}{\includegraphics[viewport=45 39 595 812]{12570f30.eps}} \end{figure}$	Figure A.22: Fits of observed spectra of DAHs from the SDSS to centered magnetic dipoles with a polar field strength $B_{\rm p}$ ( left) and dipoles shifted by $z_{\rm off}$ stellar radii along the dipole axis ( right).
Open with DEXTER

$\begin{figure}\par\resizebox{!}{17cm}{\includegraphics[viewport=45 39 595 812]{12570f31.eps}} \end{figure}$	Figure A.23: Fits of observed spectra of DAHs from the SDSS to centered magnetic dipoles with a polar field strength $B_{\rm p}$ ( left) and dipoles shifted by $z_{\rm off}$ stellar radii along the dipole axis ( right).
Open with DEXTER

$\begin{figure}\par\resizebox{17cm}{!}{\includegraphics[viewport=45 511 595 812]{12570f32.eps}} \end{figure}$	Figure A.24: Fits of observed spectra of DAHs from the SDSS to centered magnetic dipoles with a polar field strength $B_{\rm p}$ ( left) and dipoles shifted by $z_{\rm off}$ stellar radii along the dipole axis ( right).
Open with DEXTER

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.