EDP Sciences
Free Access
Issue
A&A
Volume 552, April 2013
Article Number A56
Number of page(s) 45
Section Interstellar and circumstellar matter
DOI https://doi.org/10.1051/0004-6361/201219929
Published online 25 March 2013

Online material

Appendix A: Observational details

Table A.1

Observing modes, identities, and pipeline versions for the sources sample.

Table A.2

H2O and [OI] fluxes of the intermediate-mass sources in units of 10-16  W  m-2 measured on the full 5 by 5 array.

Table A.3

Resulting fluxes in units of 10-16  W  m-2 in the spaxel with the strongest continuum (assumed to contain the central source position), corrected by the spillover factor (0.70 at 79  μm, 0.69 at 84  μm, 0.62 at 119  μm, and 0.49 at 163  μm).

Table A.4

Resulting fluxes in units of 10-16  W  m-2 in the 3 by 3 central spaxels.

Table A.5

Resulting fluxes in units of 10-16  W  m-2 on the total 5 by 5 detector array.

Appendix B: OH maps

thumbnail Fig. B.1

Maps of the OH emission from NGC 1333 IRAS 2A. The red and blue dashed lines indicate the rest wavelengths of the OH and CO transitions, respectively.

Open with DEXTER

thumbnail Fig. B.2

Maps of the OH emission from NGC 1333 IRAS 4A. The red and blue dashed lines indicate the rest wavelengths of the OH and CO transitions, respectively. Spaxels in gray were not included in the flux measurement.

Open with DEXTER

thumbnail Fig. B.3

Maps of the OH emission from NGC 1333 IRAS 4B. The red and blue dashed lines indicate the rest wavelengths of the OH and CO transitions, respectively. Spaxels in gray were not included in the flux measurement.

Open with DEXTER

thumbnail Fig. B.4

Maps of the OH emission from L 1527. The red and blue dashed lines indicate the rest wavelengths of the OH and CO transitions, respectively.

Open with DEXTER

thumbnail Fig. B.5

Maps of the OH emission from Ced 110 IRS 4. The red and blue dashed lines indicate the rest wavelengths of the OH and CO transitions, respectively.

Open with DEXTER

thumbnail Fig. B.6

Maps of the OH emission from IRAS 15398. The red and blue dashed lines indicate the rest wavelengths of the OH and CO transitions, respectively.

Open with DEXTER

thumbnail Fig. B.7

Maps of the OH emission from L 483. The red and blue dashed lines indicate the rest wavelengths of the OH and CO transitions, respectively.

Open with DEXTER

thumbnail Fig. B.8

Maps of the OH emission from Ser SMM1. The red and blue dashed lines indicate the rest wavelengths of the OH and CO transitions, respectively. See also Goicoechea et al. (2012).

Open with DEXTER

thumbnail Fig. B.9

Maps of the OH emission from Ser SMM3. The red and blue dashed lines indicate the rest wavelengths of the OH and CO transitions, respectively. Spaxels in gray were not included in the flux measurement.

Open with DEXTER

thumbnail Fig. B.10

Maps of the OH emission from L 723. The red and blue dashed lines indicate the rest wavelengths of the OH and CO transitions, respectively.

Open with DEXTER

thumbnail Fig. B.11

Maps of the OH emission from L 1489. The red and blue dashed lines indicate the rest wavelengths of the OH and CO transitions, respectively.

Open with DEXTER

thumbnail Fig. B.12

Maps of the OH emission from TMR 1. The red and blue dashed lines indicate the rest wavelengths of the OH and CO transitions, respectively.

Open with DEXTER

thumbnail Fig. B.13

Maps of the OH emission from TMC 1A. The red and blue dashed lines indicate the rest wavelengths of the OH and CO transitions, respectively.

Open with DEXTER

thumbnail Fig. B.14

Maps of the OH emission from TMC 1. The red and blue dashed lines indicate the rest wavelengths of the OH and CO transitions, respectively.

Open with DEXTER

thumbnail Fig. B.15

Maps of the OH emission from HH 46. The red and blue dashed lines indicate the rest wavelengths of the OH and CO transitions, respectively.

Open with DEXTER

thumbnail Fig. B.16

Maps of the OH emission from RNO 91. The red and blue dashed lines indicate the rest wavelengths of the OH and CO transitions, respectively.

Open with DEXTER

thumbnail Fig. B.17

Maps of the OH emission from AFGL 490. The red and blue dashed lines indicate the rest wavelengths of the OH and CO transitions, respectively.

Open with DEXTER

thumbnail Fig. B.18

Maps of the OH emission from NGC 2071. The red and blue dashed lines indicate the rest wavelengths of the OH and CO transitions, respectively.

Open with DEXTER

thumbnail Fig. B.19

Maps of the OH emission from Vela IRS 17. The red and blue dashed lines indicate the rest wavelengths of the OH and CO transitions, respectively.

Open with DEXTER

thumbnail Fig. B.20

Maps of the OH emission from Vela IRS 19. The red and blue dashed lines indicate the rest wavelengths of the OH and CO transitions, respectively.

Open with DEXTER

thumbnail Fig. B.21

Maps of the OH emission from NGC 7129. The red and blue dashed lines indicate the rest wavelengths of the OH and CO transitions, respectively.

Open with DEXTER

thumbnail Fig. B.22

Maps of the OH emission from L 1641. The red and blue dashed lines indicate the rest wavelengths of the OH and CO transitions, respectively.

Open with DEXTER


© ESO, 2013

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