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Erratum
This article is an erratum for:
[https://doi.org/10.1051/0004-6361/201117910]

Table 5

Aperture flux of observed bow shocks (Class I and II) and detached rings (Class III).

IRAS id Object Class Radiusa Dust annulus Flux (Jy) Mdust + gasb (10-2M⊙) M ISM c M ISM d
(′′) (pc) (′′) 70 μm 160 μm 70 μm 160 μm (10-4M⊙) (10-4M⊙)
00248+3518 AQ And I+III 52 0.21 40–62 (circle) 2.20  ±  0.01 1.28  ±  0.01 19.4 16.3 1.1 4.4
01159+7220 S Cas III 50e 0.23 32–64 2.26  ±  0.01 1.11  ±  0.02 26.0 18.5 12 54
01246-3248 R Scl I 54j 0.10 51–68 (arc) 1.27  ±  0.01 0.49  ±  0.01 1.4 0.8 0.1 0.3
III 14f 0.03
02168-0312 o Cet I 82j 0.04 70–150 (arc) 47.64  ±  0.03 9.75  ±  0.05 5.2 1.5 0.5 0.2
03374+6229 U Cam III 7f 0.02
II 57/62i 0.12/0.13 80–140 2.87  ±  0.02 2.44  ±  0.05 6.9 8.5 40 1110
03507+1115 NML Tau I 85 0.10 95–130 (arc) 5.23  ±  0.02 3.04  ±  0.03 4.1 3.4 3.5 62
04459+6804 ST Cam II 67/84i 0.14/0.17 84–122 1.28  ±  0.02 0.61  ±  0.03 2.9 2.0 3.1 2.2
05028+0106 W Ori I/III 92 0.17 70–120 1.99  ±  0.02 0.62  ±  0.03 3.7 1.7 8.2 32
05418-4628 W Pic I 34j 0.08 62–90 0.78  ±  0.01 0.25  ±  0.02 2.6 1.2 2.7 13
05524+0723 α Oril I 397j 0.25 510–660 (arc) 56.68  ±  0.19 22.64  ±  0.38 28.5 16.5 64 155
06331+3829 UU Aur I 82j 0.14 100–140 (arc) 5.44  ±  0.02 2.50  ±  0.03 8.2 5.4 14 88
09448+1139 R Leo I 93j 0.03 94–134 6.31  ±  0.02 1.92  ±  0.03 0.4 0.2 0.1 2.1
09452+1330 CW Leok I 507j 0.29 560–710 (arc) 6.88  ±  0.08 11.13  ±  0.11 1.3 3.0 76 31
6.00  ±  0.13 1.6
10329-3918 U Ant III 42 0.06 30–55 (circle) 16.32  ±  0.01 4.68  ±  0.01 15.2 6.3 0.4 5.3
10350-1307 U Hya I+III 114 0.12 100–133 (circle) 17.44  ±  0.03 9.33  ±  0.03 9.8 7.6 1.7 0.03
10416+6740 VY UMa II 38/46i 0.07/0.09 38–88 3.60  ±  0.01 2.33  ±  0.02 6.7 6.3 0.7 2.5
10580-1803 R Crt II  ~140 0.18 165–270 5.07  ±  0.07 6.42  ±  0.11 4.5 8.2 21 58
12427+4542 Y CVn III  ~190 0.30 150–260 5.14  ±  0.07 3.79  ±  0.10 6.9 7.3 7.7 2.9
13001+0527 RT Vir I 50–140 (circle) 5.15  ±  0.03 3.30  ±  0.04 1.2 1.1 0.6
13269-2301 R Hya I 96j 0.05 200–245 (arc) 4.65  ±  0.02 1.93  ±  0.03 0.9 0.6 3.8 12
13462-2807 W Hya III 68,230g 0.03, 0.12 70–108 (ellipse) 21.28  ±  0.02 6.08  ±  0.03 3.0 1.2 0.2 0.1
14003-7633 θ Aps I 76j 0.04 118–146 (arc) 2.15  ±  0.01 0.76  ±  0.02 0.4 0.2 1.3 0.4
15094-6953 X Tra III 150h 0.18 60–210 9.70  ±  0.08 6.89  ±  0.12 16.3 16.7 106 21
16011+4722 X Her I 45j 0.03 40–90 (ellipse) 9.17  ±  0.01 3.23  ±  0.02 2.2 1.1 0.2 0.2
17389-5742 V Pav II 97/100i 0.17/0.18 95–140 1.30  ±  0.03 1.50  ±  0.04 2.3 3.8 21 12
18476-0758 S Sct III 70 0.13 30–90 (circle) 14.09  ±  0.02 8.85  ±  0.03 27.2 24.7 13
19126+3247 W Aql II 45/75i 0.07/0.12 36–86 (ellipse) 11.10  ±  0.02 4.25  ±  0.03 16.6 9.2 5.8 144
19233+7627 UX Dra II 76/54i 0.14/0.10 50–110 2.89  ±  0.01 1.11  ±  0.03 5.6 3.1 4.4 2.5
19314-1629 AQ Sgr I 57 0.09 50–100 3.44  ±  0.02 2.53  ±  0.02 4.9 5.3 5.4 3.7
19390+3229 TT Cyg III 33 0.07 26–43 (circle) 1.74  ±  0.01 0.86  ±  0.01 4.3 3.1 1.3 21
20038-2722 V1943 Sgr I 66j 0.06 50–130 (arc) 5.98  ±  0.03 2.30  ±  0.03 3.0 1.7 2.6 0.8
20075-6005 X Pav I 50j 0.07 94–122 5.74  ±  0.01 2.69  ±  0.02 4.4 2.3 3.1 19
20141-2128 RT Cap III 92 0.13 62–118 2.21  ±  0.02 0.91  ±  0.04 2.4 1.4 4.0 15
20248-2825 T Mic I 40–100 (ellipse) 5.48  ±  0.02 0.58  ±  0.03 3.2 0.5 1.2
21358+7823 S Cep III 90 0.18 70–130 2.14  ±  0.03 4.6 11 142
21419+5832 μ Cep I 78j 0.15 100–150 28.64  ±  0.04 11.5  ±  0.12 56.4 32.8 56 637
21439-0226 EP Aqr I 43j 0.03 45–68 3.68  ±  0.01 0.99  ±  0.01 0.6 0.2 0.1 1.2
23438+0312 TX Psc III 16f 0.02
I 38j 0.05 12–58 (ellipse) 4.79  ±  0.01 1.07  ±  0.02 4.7 1.5 0.2 0.7
23558+5106 R Cas I 97j 0.06 100–160 (arc) 8.35  ±  0.01 3.52  ±  0.04 1.7 1.1 2.5 2.9

Notes. Irregular Class IV is excluded.

(a)

Radii of rings and fermata derived from the azimuthally averaged radial profiles (Fig. 1).

(b)

Derived from Eq. (1) using the total integrated flux at 70 and 160 μm, respectively, adopting a gas-to-dust ratio of 200 and a dust temperature of 30 K.

(c)

MISM = , with nH taken from Eq. (5).

(d)

MISM, with nH taken from the local densities inferred from the measured stand-off distance and Eq. (2); Tables 1 and 2.

(e)

Central source is offset by 0′′ RA, 5′′ Dec.

(f)

Ring radius from the deconvolved image.

(g)

Inner and outer (at 160 μm) rings, respectively.

(h)

Central source is offset by 12′′ RA, 5′′ Dec.

(i)

Radial distances are quoted for both north and south arcs (east-west for W Aql).

(j)

Projected distance A (Fig. 6).

(k)

CW Leo has been observed two times at 160 μm.

(l)

Updated distance to 197 pc (Harper et al. 2008).

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