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This article has an erratum: [https://doi.org/10.1051/0004-6361/201833177e]

Table D.2.

Stellar and circumstellar information taken from the bibliography for the objects of the sample.

Target name Variability Teff (K) d (pc) vexp (km s−1) ṀBibliography (M⊙ yr−1) References
RR Aql Mira 2000 530 9.0 2.4 × 10−6 (0.9,6.2) × 10−6 7, 34
9.1 × 10−7
Omi Cet Mira 2200 110 8.1 2.5 × 10−7 (0.2,1.2) × 10−6 18, 29, 34
5 × 10−7
W Hya SRa 2200 98 7.0 1.5 × 10−7 (0.3,3.8) × 10−7 10, 12, 18, 23, 32, 34
7.8 × 10−8
10−7
7 × 10−8
8.1 × 10−8
IRAS 20038-2722 SRb 2200 197 5.4 9.9 × 10−8 (0.7,3.9) × 10−7 7, 14, 32
1.3 × 10−7
T Cep Mira 2400 190 5.5 9.1 × 10−8 (0.8,2.4) × 10−7 7
NML Tau Mira 2700 260 19.0 5 × 10−6 (0.2,3.5) × 10−5 3, 10, 18, 19, 23, 27, 34
8 × 10−6
2 × 10−5
4.5 × 10−6
10−5
4.7 × 10−6
4.4 × 10−6
R Dor SRb 2800 59 5.7 1.6 × 10−7 (0.9,4.2) × 10−7 1, 3, 10, 23, 32, 34
2 × 10−7
1.3 × 10−7
6.9 × 10−8
TX Cam Mira 2800 380 18.5 4 × 10−6 (0.2,1.5) × 10−5 3, 10, 18, 23, 24
5.5 × 10−6
7 × 10−6
6.5 × 10−6
X Her SRV 2800 137 6.5 1.5 × 10−7 (0.8,2.6) × 10−7 14, 32, 34
10−6
IRAS 19474-0744 SR 2800 810a 13.6 4.1 × 10−6 (0.5,1.6) × 10−5 34,35
T Mic SRb 2800 290 4.8 8 × 10−8 (1.9,6.9) × 10−7 29, 32, 34
2.7 × 10−7
R Cas Mira 3100 176 10.5 8 × 10−7 (0.5,2.2) × 10−6 3, 10, 18, 23
9 × 10−7
4 × 10−7
EP Aqr SRb 3200 114 10.0 3.1 × 10−7 (0.9,5.0) × 10−7 8, 18
1.2 × 10−7
NML Cyg SRc 3800 620 33 8.7 × 10−5 (0.6,2.3) × 10−4 18, 35
1.8 × 10−6
χ Cyg Mira 2000 149 8.5 7 × 10−7 (0.1,1.2) × 10−6 10, 17, 18, 20, 27
4 × 10−7
2.4 × 10−7
π Gru SRb 2300 152 10.0 8.5 × 10−7 (1.6,4.9) × 10−7 2, 7, 18
7.7 × 10−7
W Aql Mira 2800 395 16.5 2.7 × 10−6 (0.2,1.2) × 10−5 10, 11, 18, 21, 28
1.3 × 10−5
2.2 × 10−6
2.5 × 10−6
4 × 10−6
WX Psc Mira 2000 700 19.3 1.7 × 10−5 (0.4,6.9) × 10−5 10, 13, 18, 26, 35
4 × 10−5
1.9 × 10−5
6 × 10−6
8.5 × 10−6
V1300 Aql Mira 2000 620 16.5 10−5 (0.4,3.3) × 10−5 7, 10, 18, 24
4.5 × 10−6
1.6 × 10−5
OH 231.8+4.2 Mira 2500 1500 15.0 1.6 × 10−4 (0.9,2.8) × 10−4 15, 33
OH 26.5+0.6 Mira 2750 1370 17.0 1.0 × 10−4 (3,0.8) × 10−4 13, 18
9.7 × 10−6
IRAS 22036+5306 No 6900 4000 30.0 7.5 × 10−5 (0.04,1.3) × 10−4 16
7 × 10−6
AFGL 6815 No 7000 2900 15.0 2.1 × 10−5 (1.3,4.7) × 10−5 5, 9, 18, 31
3 × 10−5
IRAS 17347-3139 No 30000a 3680a 25.0 – – 5, 30
NGC 6537 No 200000 1500 18.0 – – 31
NGC 6302 No 250000 1170 10.0 1.5 × 10−4 (0.09,3.6) × 10−4 4, 6, 22, 25
2.7 × 10−5

Notes. Column 1: target name; Col. 2: variability of the central star; Col. 3: effective temperature of the star; Col. 4: adopted distance to the object; Col. 5: expansion velocity of the circumstellar envelope; Col. 6: left: mass loss rate taken from the literature. Right: range of mass loss rates shown at left after being scaled to the values of d, vexp and χCO used in this work. For those with only one previous estimation, the range cover a factor of 3 around that value after scaling.

(a)

Uncertain.

References. (1) Van de Sande et al. (2018) (2) Doan et al. (2017) (3) Maercker et al. (2016), (4) Santander-García et al. (2015), (5) Vickers et al. (2015), (6) Santander-García et al. (2015), (7) Danilovich et al. (2015), (8) Nhung et al. (2015), (9) He et al. (2014), (10) Ramstedt & Olofsson (2014), (11) Danilovich et al. (2014), (12) Khouri et al. (2014), (13) Justtanont et al. (2013), (14) Cox et al. (2012), (15) Choi et al. (2012), (16) Sánchez Contreras & Sahai (2012), (17) Schöier et al. (2011), (18) De Beck et al. (2010), (19) Decin et al. (2010), (20) Justtanont et al. (2010), (21) Ramstedt et al. (2009), (22) Meaburn et al. (2008), (23) Maercker et al. (2008), (24) Ramstedt et al. (2008), (25) Dinh-V-Trung et al. (2008), (26) Decin et al. (2007), (27) Teyssier et al. (2006), (28) Ramstedt et al. (2006), (29) Heras & Hony (2005), (30) Matsuura et al. (2005), (31) Woods et al. (2005), (32) Olofsson et al. (2002), (33) Alcolea et al. (2001), (34) Loup et al. (1993) and (35) Knapp et al. (1982).

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