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Table 4

Total H I and FIR (H I + H2 + dust) masses of CSEs.

Name Var. Spec. Teff (K) MHI (M) M60μm (M) M60MHI$\[\frac{M_{60}}{M H I}\]$ M70μm (M) M160μm (M) M70MHI$\[\frac{M_{70}}{M H I}\]$
—IRAS— ———-Herschel———
Clear H I detections
R Cas Mira M6.5-9e 3129 0.0047 0.0843 17.9 0.0255 0.0165 5.4
o Cet Mira M5-9IIIe+DA 2500 0.0009 0.0777 86.4 0.0416 0.0120 46.0
R Hya Mira M6-9e 2128 0.0034 0.0339 10.0 0.0072 0.0048 2.1
RS And SRa ... ... 0.0186 0.0974 5.2 ... ... ...
RW Boo SRb M5III: 3148 0.0272 0.0080 0.3 ... ... ...
Y CVn SRb C-N5 2760 0.0759 0.2650 3.5 0.1287 0.1362 1.7
S Dra SRb M6III ... 0.0096 0.0412 4.3 ... ... ...
RY Dra SRb: C-N3III: 2810 0.1264 0.2874 2.3 ... ... ...
X Her SRb M6III 3281 0.0099 0.0089 0.9 0.0142 0.0071 1.4
U Hya SRb C-N5 2965 0.0015 0.5386 359.0 0.1960 0.1520 130.7
Y Uma SRb M7II-III: ... 0.0147 0.0316 2.2 ... ... ...
BK Vir SRb M7-III: 3074 0.0026 0.0158 6.1 ... ... ...
RT Vir SRb M8III 2602 0.0115 0.0380 3.3 0.0304 0.0279 2.6
μ Cepa SRc M2-Ia 3700 0.0413 ... ... 1.2189 0.7088 29.5
TX Psc Lb C-N6 3125 0.0069 0.0696 10.1 ... ... ...
V1942 Sgr Lb C-N5+ 2960 0.3681 0.3326 0.9 ... ... ...
V1943 Sgr Lb M7/8III 2752 0.0269 0.0308 1.1 0.0240 0.0136 0.9
VY UMa Lb C-N5 2930 0.0099 0.0773 7.8 0.1637 0.1539 16.5
Possible H I detections
UX Dra SRa: C-N5 3090 0.0078 0.1196 15.3 0.1661 0.0919 21.3
SV Peg SRb M7 ... 0.0109 0.0185 1.7 ... ... ...
AQ Sgr SRb C-N5 2790 0.1012 0.2719 2.7 0.2742 0.2966 2.7
EP Aqr SRb M7-III: 3236 0.0005 0.0101 20.2 0.0062 0.0021 12.5
RS Cnc SRc M6S 3214 0.0022 0.0074 3.4 ... ... ...
Sources with H I upper limits
W Aql Mira S6/6e 2800 <0.0095 ... ... 0.2009 0.1113 >18.1
IK Tau (NRT) Mira M7-11 2667 <0.0091 ... ... 0.0371 0.0309 >5.5
IK Tau (VLA) <0.0028 >13.3
RS And SRa ... ... <0.0186 0.0974 >5.2 ... ... ...
W Hya (VLA) SRa M 2400 <0.0017 ... ... 0.0598 0.0239 >35.7
RT Cap SRb C6.4 2485 <0.0125 0.2470 >19.8 0.1755 0.1024 >14.0
RV Cyg SRb C-N5: 2675 <0.1055 0.6942 >6.6 ... ... ...
T Mic SRb M77/8III 2856 <0.0045 0.0275 >6.1 0.0198 0.0031 >4.4
R Sclb SRb C-N5+ 2295 <0.0125 0.2428 >19.4 0.0514 0.0295 >4.1
U Ant Lb C-N3 2775 <0.0477 0.3045 >6.4 0.3238 0.1342 >6.8
Confused NRT sources detected with the VLA
IRC+10216 Mira C9.5 2200 0.0032 0.7699 240.1 (0.19) ... (59.4)

Notes. a: μ Cep is an M type supergiant, not an AGB star. b: for R Scl the masses are based on the Herschel FIR flux densities listed here and a distance of 370 pc, whereas Cox et al. (2012b) used a distance of 290 pc. Herschel FIR values are from Cox et al. (2012b), except for IRC+10216, whose total gas + dust mass is based on 100 μm Herschel data from Decin et al. (2011). For Teff references, see Table A.1.

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