Free Access
Volume 563, March 2014
Article Number A87
Number of page(s) 20
Section Interstellar and circumstellar matter
Published online 14 March 2014

Online material

Appendix A: Additional materials

thumbnail Fig. A.1

Proper motions of the knots in the HH 409 jet. Same as Fig. 2; the dash-dotted lines correspond to the best global fit made to the positions of the knots, with parameters 16.0 ± 0.7 yr and proper motions vt,red = 0.28 ± 0.01′′ yr-1, and vt,blue = 0.49 ± 0.01′′ yr-1. The A2 data are omitted from the fitting procedure.

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thumbnail Fig. A.2

Lightcurve of HD 163296 compiled from the resources listed in Table A.1. The dotted lines indicate the mean values. References for plot symbols: (1) de Winter et al. (2001); (2) Manfroid et al. (1991); (3) Maidanak Observatory (Grankin et al., in prep.); (4) Swiss (this work); (5) Perryman et al. (1997); (6) Hillenbrand et al. (1992); (7) Eiroa et al. (2001) (8) Pojmanski & Maciejewski (2004); (9) AAVSO (this work); (10) Tannirkulam et al. (2008b); (11) Mendigutía et al. (2013); (12) Sitko et al. (2008); (13) de Winter et al. (2001); (14) Berrilli et al. (1992); (15) BASS; (16) SpeX (Sitko et al. 2008, this work); (17) Kimeswenger et al. (2004); (18) Skrutskie et al. (2006).

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Table A.1

Overview of datasets used in this study.

Table A.2

Mass accretion rate from Brγ luminosity.

© ESO, 2014

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