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This article has an erratum: [https://doi.org/10.1051/0004-6361/201117910e]

Table 3

AGB stars that show no obvious bow shocks are assigned to Class X pending further notice.

IRAS identifier Name DistanceA Ṁ z23 μ v⋆ PA i Predicted TypeI Binary
(pc) (10-7M⊙ yr-1) (pc) (cm-3) (mas yr-1) (km s-1) (° N-E) (°) (km s-1) (′) (pc)
X “Non-detection”
01037+1219 WX Psc 7401 1902, 7724 –553 0.01  ≥ 9.0 19.82  ≤ 9.5  ≤ 2.0 O-M9
01144+6658 AFGL 190 279014 63814 37 1.38  ≥ 21.0 18.113 C
01304+6211 OH 127.8+0.0 210023 50023 14 1.73  ≥ 55.3 12.523  ≤ 1.1  ≤ 0.7 O
02270-2619 R For 69013 9.024 –625 0.00 6.9 22.6 120.8 –5 16.116  ≤ 0.8  ≤ 0.2 C
03112-5730 TW Hor 322  ±  38h 1.524, 0.2414 265 0.14 34.3 52.4 58.8 1 7.515 0.5 0.05 C yes2
04020-1551 V Eri 439  ±  133h –290 0.11 16.7 39.8 205.6 –31 1325 0.9 0.12 O M5/M6IV yes2
04361-6210 R Dor 55  ±  3h 6.124, 1.317 –20 1.64 146.4 39.4 217.1 10 6.017 4.8 0.08 O M8IIIe yes1
04566+5606 TX Cam 3802 652,3424 72 0.98  ≥ 10.8 21.22  ≤ 10.7  ≤ 1.2 O-M8.5 yes13
04573-1452 R Lep 413  ±  174h 1324 –200 0.27 6.5 18.5 116.5 42 17.46 2.9 0.35 C
07209-2540 VY CMa 114027, 562 28002 –35 1.41 12.4 42.9 86.9 36 46.52 31.0 5.1 O-M3/M4III yes1
09076+3110 RS Cnca 143  ±  11h, 12228 27-36/ 0.55-0.7413 111 0.66 18.3 14.1 154.4 30 8.06 2.7 0.11 O-M6IIIaeS
10131+3049 RW LMi 32014, 4401 19.2, 592 384 0.04  ≥ 1.6 20.82  ≤ 71.8  ≤ 9.2 C
10491-2059 V Hya 60014 2.824,83.1,6102 399 0.04 7.2 27.9 302.3 –38 302 7.8 1.6 C yes11
11331-1418 HD100764 290  ±  83h 218 0.23 17.6 24.3 126.6 1 2.2 0.2 C
12544+6615 RY Dra 431  ±  110h 2.124 351 0.06 23.6 49.2 116.8 –9 10.015 0.4 0.05 C
14219+2555 RX Boo 190  ±  23h 3.62,6.224 193 0.29 58.7 52.9 142.9 2 9.02 1.3 0.07 O-M7.5
15194-5115 II Lup 59014, 5002 18124, 392 56 1.15  ≥ 15.0 232  ≤ 6.5  ≤ 0.9 C
15477+3943 V CrB 63013 7.124 506 0.01 15.5 114.2 151.9 –64 8.113 0.02 0.02 C
18050-2213 VX Sgr 262  ±  187h 6102, 14024 10 1.80 4.1 8.5 28.1 50 24.32 31.6 2.4 O-M4eIa yes1
18240+2326 AFGL 2155 92014 45.614 265 0.14  ≥ 60.0 16.125 C
18306+3657 T Lyr 719  ±  254h,65026 9.414, 0.715 232 0.20 8.5 26.8 225.8 17 11.515 0.24 0.05 C
18348-0526 OH 26.5+0.6 13702 972, 35024 30 1.49  ≥ 27.4 17.02  ≤ 1.8  ≤ 0.7 O
20077-0625 IRC-10 529 6202 452, 9024 –201 0.27  ≥ 18.0 16.52  ≤ 5.6  ≤ 1.0 O
21197-6956 Y Pav 403  ±  96h 1.615 –234 0.19 2.9 5.8 124.0 –44 8.015 7.3 0.86 C
23166+1655 LL Peg 100014, 9802 14414, 3102 –620 0.00  ≥ 31.0 16.02  ≤ 3.8  ≤ 1.1 C yes12
23320+4316 LP And 78014, 6302 462, 15015 –171 0.36  ≥ 17.0 14.02  ≤ 3.9  ≤ 0.7 C
NML Cyg 12202 8702, 35024 –26 1.54  ≥ 2.0 33.02  ≤ 71.5  ≤ 25.4 O-M6IIIe
07245+4605 Y Lyn 253  ±  61h 5.613/0.3613 123 0.58 11.5 13.9 32.6 –2 5.413 4.1 0.3 O-M6SIb-II yes15
13114-0232 SW Vir 143  ±  17h 1.4x, 4t 138 0.50 15.8 14.7 301.5 –49 7.8a, 7.5t 1.4 0.06 O-M7III
17411-3154 AFGL 5379 11902,h 2802, 350x –13 1.76  ≥ 22.7 25.02  ≤ 5.4  ≤ 1.9 O

Notes. Notes and references as in Table 1. Note that Y Lyn, SW Vir, and AFGL 5379 are classified X pending planned observations.

(a)

The central source is possible extended. However, no detached emission is detected.

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