RACE-OC project: Rotation and variability of young stellar associations within 100 pc

Free Access

Issue		A&A Volume 520, September-October 2010


Article Number		A15
Number of page(s)		63
Section		Stellar structure and evolution
DOI		https://doi.org/10.1051/0004-6361/200913644
Published online		22 September 2010

Online Material

Table A.1: TW Hydrae association.

Table A.2: $\beta$ Pictoris association.

Table A.3: Tucana/Horologium association.

Table A.4: Columba association.

Table A.5: Carina association.

Table A.6: AB Doradus association.

Table A.7: Summary of period search.

$\begin{figure} \par\mbox{\includegraphics[angle=0,width=7.5cm,height=5.0cm,clip]... ...degraphics[angle=0,width=7.5cm,height=5.0cm,clip]{644f37.ps} } \par \end{figure}$

Figure A.1:

ASAS V-band light curves of TW Hydrae (confirmed and rejected) members. Top panel: V-band data time series, where different colour are used to mark different time intervals. second panel from top: rotation period vs. time detected with a confidence level over 99%; third panels: periodogram ( left) and spectral window function ( right). Horizontal line indicate the power level corresponding to a 99% confidence level. Vertical solid line in the periodogram indicates the peak corresponding to the adopted rotation period. Bullets are beats of the rotation period. The vertical dotted line indicates that rotation period differs from the period at the spectral window function maximum. Bottom panel: light curve phase with the adopted rotation period. Solid line is a sinusoidal fit with the rotation period.

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$\begin{figure} \par\mbox{\includegraphics[angle=0,width=9cm,height=6.0cm,clip]{6... ...\includegraphics[angle=0,width=9cm,height=6.0cm,clip]{644f41.ps} }\end{figure}$	Figure A.2: TWA members: continued from Fig. A.1.
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$\begin{figure} \par\mbox{\includegraphics[width=8cm,height=6.0cm,clip]{644f42.ps... ...4f48.ps}\includegraphics[width=8cm,height=6.0cm,clip]{644f49.ps} }\end{figure}$	Figure A.3: ASAS V-band light curves of $\beta$ Pictoris members. See Fig. A.1 for explanation.
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$\begin{figure} \mbox{ \psfig{file=644f50.ps,width=9cm,height=6.0cm,angle=0}\psfi... ...cm,angle=0}\psfig{file=644f57.ps,width=9cm,height=6.0cm,angle=0} }\end{figure}$	Figure A.4: $\beta$ Pictoris members: continued from Fig. A.3.
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$\begin{figure} \mbox{ \psfig{file=644f58.ps,width=9cm,height=6.0cm,angle=0}\psfi... ...cm,angle=0}\psfig{file=644f65.ps,width=9cm,height=6.0cm,angle=0} }\end{figure}$	Figure A.5: $\beta$ Pictoris members: continued from Fig. A.4.
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$\begin{figure} \mbox{ \psfig{file=644f66.ps,width=9cm,height=6.0cm,angle=0} }\end{figure}$	Figure A.6: $\beta$ Pictoris members: continued from Fig. A.5.
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$\begin{figure} \mbox{ \psfig{file=644f67.ps,width=9cm,height=6.0cm,angle=0}\psfi... ...cm,angle=0}\psfig{file=644f74.ps,width=9cm,height=6.0cm,angle=0} }\end{figure}$	Figure A.7: ASAS V-band light curves of Tucana/Horologium members. See Fig. A.1 for explanation.
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$\begin{figure} \mbox{ \psfig{file=644f75.ps,width=9cm,height=6.0cm,angle=0}\psfi... ...cm,angle=0}\psfig{file=644f82.ps,width=9cm,height=6.0cm,angle=0} }\end{figure}$	Figure A.8: Tucana/Horologium members: continued from Fig. A.7.
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$\begin{figure} \mbox{ \psfig{file=644f83.ps,width=9cm,height=6.0cm,angle=0}\psfi... ...cm,angle=0}\psfig{file=644f89.ps,width=9cm,height=6.0cm,angle=0} }\end{figure}$	Figure A.9: Tucana/Horologium members: continued from Fig. A.8.
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$\begin{figure} \mbox{ \psfig{file=644f90.ps,width=9cm,height=6.0cm,angle=0}\psfi... ...ig{file=644f92.ps,width=9cm,height=6.0cm,angle=0}\hspace*{4.5cm} }\end{figure}$	Figure A.10: Tucana/Horologium members: continued from Fig. A.9.
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$\begin{figure} \mbox{ \psfig{file=644f93.ps,width=9cm,height=6.0cm,angle=0}\psfi... ...m,angle=0}\psfig{file=644f100.ps,width=9cm,height=6.0cm,angle=0} }\end{figure}$	Figure A.11: ASAS V-band light curves of Columba members. See Fig. A.1 for explanation.
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$\begin{figure} \mbox{ \psfig{file=644f101.ps,width=9cm,height=6.0cm,angle=0}\psf... ...gle=0}\psfig{file=644f108.ps,width=9cm,height=6.0cm,angle=0} } \par \end{figure}$	Figure A.12: Columba members: continued from Fig. A.11.
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$\begin{figure} \par\mbox{ \psfig{file=644f109.ps,width=9cm,height=6.0cm,angle=0}\psfig{file=644f110.ps,width=9cm,height=6.0cm,angle=0} } \par \end{figure}$	Figure A.13: Columba members: continued from Fig. A.12.
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$\begin{figure} \par\mbox{ \psfig{file=644f111.ps,width=9cm,height=6.0cm,angle=0}... ...gle=0}\psfig{file=644f117.ps,width=9cm,height=6.0cm,angle=0} } \par \end{figure}$	Figure A.14: ASAS V-band light curves of Carina members. See Fig. A.1 for explanation.
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$\begin{figure} \par\mbox{ \psfig{file=644f118.ps,width=9cm,height=6.0cm,angle=0}... ...gle=0}\psfig{file=644f125.ps,width=9cm,height=6.0cm,angle=0} } \par \end{figure}$	Figure A.15: Carina members: continued from Fig. A.14.
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$\begin{figure} \par\mbox{ \psfig{file=644f126.ps,width=9cm,height=6.0cm,angle=0}... ...gle=0}\psfig{file=644f129.ps,width=9cm,height=6.0cm,angle=0} } \par \end{figure}$	Figure A.16: Carina members: continued from Fig. A.15.
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$\begin{figure} \par\mbox{ \psfig{file=644f130.ps,width=9cm,height=6.0cm,angle=0}... ...gle=0}\psfig{file=644f137.ps,width=9cm,height=6.0cm,angle=0} } \par \end{figure}$	Figure A.17: ASAS V-band light curves of AB Doradus members. See Fig. A.1 for explanation.
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$\begin{figure} \par\mbox{ \psfig{file=644f138.ps,width=9cm,height=6.0cm,angle=0}... ...gle=0}\psfig{file=644f145.ps,width=9cm,height=6.0cm,angle=0} } \par \end{figure}$	Figure A.18: AB Doradus members: continued from Fig. A.17.
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$\begin{figure} \par\mbox{ \psfig{file=644f146.ps,width=9cm,height=6.0cm,angle=0}... ...gle=0}\psfig{file=644f153.ps,width=9cm,height=6.0cm,angle=0} } \par \end{figure}$	Figure A.19: AB Doradus members: continued from Fig. A.18.
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$\begin{figure} \par\mbox{ \psfig{file=644f154.ps,width=9cm,height=6.0cm,angle=0}... ...gle=0}\psfig{file=644f161.ps,width=9cm,height=6.0cm,angle=0} } \par \end{figure}$	Figure A.20: AB Doradus members: continued from Fig. A.19.
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$\begin{figure} \par\mbox{ \psfig{file=644f162.ps,width=9cm,height=6.0cm,angle=0}... ...gle=0}\psfig{file=644f169.ps,width=9cm,height=6.0cm,angle=0} } \par \end{figure}$	Figure A.21: AB Doradus members: continued from Fig. A.20.
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$\begin{figure} \par\mbox{ \psfig{file=644f170.ps,width=9cm,height=6.0cm,angle=0}\psfig{file=644f171.ps,width=9cm,height=6.0cm,angle=0} } \par \end{figure}$	Figure A.22: AB Doradus members: continued from Fig. A.21.
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