| Issue |
A&A
Volume 523, November-December 2010
|
|
|---|---|---|
| Article Number | A73 | |
| Number of page(s) | 41 | |
| Section | Stellar structure and evolution | |
| DOI | https://doi.org/10.1051/0004-6361/201014763 | |
| Published online | 18 November 2010 | |
Online material
Appendix A: Companion candidates motions on the sky
The astrometric measurements for all point sources detected at several observing epochs are represented in Fig. A.1. The background/comoving probabilities defined in Sect. 4.2 are given over each panel.
 |
Fig. A.1
Motions of companion candidates measured on the sky relatively to their respective primary stars (at (Δα,Δδ) = (0,0)). The theoretical motion of an object is calculated from its initial first epoch measurement (black filled circle) assuming it is a background contaminant and given the proper and parallactic motions of the primary star (black curve), for the different epochs where measurements have been recorded (empty circles). The measured positions for these different epochs are reported (filled circles) for comparison. When the measurements (filled circles) agree with the theoretical motion path, the companion candidate is likely a background contaminant. |
| Open with DEXTER | |
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Fig. A.1
continued. |
| Open with DEXTER | |
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Fig. A.1
continued. |
| Open with DEXTER | |
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Fig. A.1
continued. |
| Open with DEXTER | |
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Fig. A.1
continued. |
| Open with DEXTER | |
Appendix B: Detection limits for all stars
 |
Fig. B.1
Detection limits in the Ks band. |
| Open with DEXTER | |
 |
Fig. B.1
continued. |
| Open with DEXTER | |
 |
Fig. B.1
continued. |
| Open with DEXTER | |
 |
Fig. B.1
continued. |
| Open with DEXTER | |
 |
Fig. B.1
continued. |
| Open with DEXTER | |
 |
Fig. B.1
continued. |
| Open with DEXTER | |
 |
Fig. B.1
continued. |
| Open with DEXTER | |
 |
Fig. B.1
continued. |
| Open with DEXTER | |
 |
Fig. B.1
continued. |
| Open with DEXTER | |
 |
Fig. B.1
continued. |
| Open with DEXTER | |
 |
Fig. B.2
Detection limits in the H band. |
| Open with DEXTER | |
 |
Fig. B.2
continued. |
| Open with DEXTER | |
 |
Fig. B.3
Detection limits in the J band. |
| Open with DEXTER | |
 |
Fig. B.3
continued. |
| Open with DEXTER | |
Appendix C: The HD 49095 triple system
 |
Fig. C.1
Orbit of the binary companion to HD 49095 resolved over 3.5 yr. The blue and red dots mark the positions of CC1 and CC2, respectively, as retrieved by the deconvolution algorithm. The axes give the projected separations with respect to CC1. |
| Open with DEXTER | |
Appendix D: HD 32743 motion over 49 years
 |
Fig. D.1
Motion of HD 32743 (η1 Pic) CC1 on the sky considering the 1946 archive values for ρ and θ in the CCDM with arbitrary uncertainties. The filled red dot indicates the position measured in 2005. This companion candidate is considered as a probable background object. |
| Open with DEXTER | |
© ESO, 2010
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