Free Access
Issue
A&A
Volume 569, September 2014
Article Number A5
Number of page(s) 22
Section Interstellar and circumstellar matter
DOI https://doi.org/10.1051/0004-6361/201424136
Published online 08 September 2014

Online material

Appendix A: Stellar properties

The stellar and accretion parameters for the GTO sample are listed in Table A.1 (see Alcalá et al. 2014; Rigliaco et al. 2012).

Table A.1

Stellar properties.

Appendix B: Line properties

Tables B.1B.4 list the properties of the LVC, HVC blueshifted, and HVC redshifted components of the lines [O i] 557.79, [O i] 630.03, [O ii] 372.60, [O ii] 731.89, [S ii] 406.86, [S ii] 673.08, and [N ii] 658.34. For each component the tables give the intensity, the uncertainty, the velocity shift of the line peak, and the FWHM of the observed component. When not detected, we give 3σ upper limit for only the LVC.

Table B.1

Fluxes, velocity peak, and full width at half maximun of [O i] lines.

Table B.2

Fluxes, velocity peak, and full width at half maximun of [O ii] lines.

Table B.3

Fluxes, velocity peak, and full width at half maximun of [S ii] lines.

Table B.4

Fluxes, velocity peak, and full width at half maximun of [N ii] lines.

Appendix C: Examples of line profiles in selected objects

In this Appendix we show examples of the line profiles discussed in this paper.

thumbnail Fig. C.1

Normalized, continuum subtracted line profile of the [O i] 630.03 line. The profiles are shifted vertically for an easier display.

Open with DEXTER

thumbnail Fig. C.2

Normalized, continuum subtracted line profiles (as labeled) for the object Sz66. In this and the following figures the dashed colored curves show the LVC (green), HVC blueshifted (blue) and HVC redshifted (red); the total is given by the dotted (black) line. In this object, only the LVC is detected.

Open with DEXTER

thumbnail Fig. C.3

Same as Fig. C.2 for Sz69.

Open with DEXTER

thumbnail Fig. C.4

Same as Fig. C.2 for Sz73.

Open with DEXTER

thumbnail Fig. C.5

Same as Fig. C.2 for Sz88A. The two panels for the lines [N ii] 658.34 and [S ii] 673.08 illustrate typical non-detections.

Open with DEXTER

thumbnail Fig. C.6

Same as Fig. C.2 for Sz99.

Open with DEXTER

thumbnail Fig. C.7

Same as Fig. C.2 for Sz100.

Open with DEXTER

thumbnail Fig. C.8

Same as Fig. C.2 for Sz106.

Open with DEXTER

thumbnail Fig. C.9

Same as Fig. C.2 for Sz113. Note that the [O i] 557.79 is a 3σ detection.

Open with DEXTER

thumbnail Fig. C.10

Same as Fig. C.2 for SO848.

Open with DEXTER


© ESO, 2014

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