Free Access
Issue
A&A
Volume 524, December 2010
Article Number A97
Number of page(s) 13
Section Galactic structure, stellar clusters and populations
DOI https://doi.org/10.1051/0004-6361/201015306
Published online 25 November 2010

Appendix A: Online material

Table A.1

Sources detected in the 0.3–7.5 keV energy band using PWDetect with detection threshold SNR = 5.

thumbnail Fig. A.1

X-ray spectra for known members of η Chamaleontis. Red is for EPIC-pn and black is for EPIC-mos, except for RECX 12 that is located in an EPIC-pn gap. The best fit to each spectrum is also plotted. The bottom panel represents the deviation of the model from the observed spectra in each spectral bin.

Open with DEXTER

thumbnail Fig. A.2

X-ray light curves in the energy band 0.3−8.0 keV for known members of η Chamaleontis. Time binning ranges from 15 to 30 min.

Open with DEXTER


© ESO, 2010

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