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Table B.1

Published integrated CO(1-0) line fluxes

Name var. Spec. <ICO,corr> published CO line fluxes, telescope diameters, and references FHI ICO,corr/FHI
(K km/s) ——————-K km/s), (m), ref.——————- (Jy km/s) (K/Jy)
Clear H I detections
R Cas Mira M 13.5 1.9 Kn85 7 14.4 Li88 20 5.2 Ma90 14 0.61 22.1
AX Cep Mira N 3.4 7.4 Gr99 30 7.8 Gr99 30 0.31 11.0
o Cet Mira M+DA 37.8 2.6 Kn85 7 9.1 Kn85 7 8.8 Ma90 14 0.45 84,0
R Gem Mira S 3.4 2.4 Ra09 20 9.7 Ra09 30 0.13 26.2
R Peg Mira M 0.3 0.7 Gr99 30 0.49 0.6
RV Boo SRb M 2.0 2.0 Ny92 20 0.37 5.4
Y CVn SRb C 4.9 2.1 Ma90 14 6.3 Ol87 20 4.5 Ol93 20 3.08 1.6
RY Dra SRb: C 2.4 2.4 Ol93 20 3.30 0.7
X Her SRb M 4.8 13 Di19 30 4.7 Ny92 20 3.9 Ke99 20 2.57 1.9
U Hya SRb C 6.8 4.7 Ol88 15 4.6 Ol93 15 8.9 Da15 30 0.14 48.6
SV Psc SRb M 3.3 1.6 Ma90 14 0.06 56.9
Y UMa SRb M 4.5 2.9 Zu89 12 0.5 Ma90 14 0.54 8.3
BK Vir SRb M 1.6 0.8 Ma90 14 3.7 Da15 30 0.21 7.6
RT Vir SRb M 10.6 1.3 Kn85 7 0.77 13.8
RS Cnc SRc M 26.0 7.3 Kn85 7 4.1 Ma90 14 22.9 Da15 30 0.41 63.4
V1942 Sgr Lb C 2.1 1.2 Ol93 20 0.82 2.6
VY UMa Lb C 1.4 1.4 Ol93 20 0.10 14.0
Possible H I detections
RAFGL 3099 Mira C 17.1 2.1 Kn85 7 0.04 380.0
GY Aql Mira M 11.4 5.6 Ma90 14 0.55 20.7
S CMi Mira M 0.1 0.6 Da15 30 0.16 0.6
WX Ser Mira M 1.8 0.4: Kn86 7 0.9 Ma90 14 0.09 20.0
UX Dra SRa: C 2.9 2.9 Ol93 20 0.14 20.7
EP Aqr SRb M 11.2 5.0 Zu86a 12 4.2 Ma90 14 0.11 101.8
S Dra SRb M 1.6 1.6 Ny92 20 0.14 11.4
AQ Sgr SRb C 2.8 1.6 Ol93 15 1.27 2.2
Sources with H I upper limits
RAFGL 865old Mira C 37.5 3.3 Kn85 7 27.0 Ny92 15 <2.40 >15.6
KU Andold Mira M 19.7 8.7 Ma90 14 48.9 Da15 30 <5.88 >3.4
W Aql Mira S 53.4 9.6 Kn85 7 28.4 Ny92 20 26.2 Ma90 14 <0.29 >184.1
V CrB Mira M 3.0 2.7 Ol93 20 7.6 Gr99 30 <0.07 >41.1
R For Mira C 7.4 3.1 Zu86a 12 4.8 Ol93 15 11.4 Gr99 30 <0.21 >35.2
X Hya Mira M <0.6 1.4 Gr99 30 <0.88 >0.7:
T Lepold Mira M <0.5 1.1 Gr99 30 <2.04 >0.2:
R LMi Mira M 0.9 2.3 Gr99 30 1.9 Bu86 30 <0.40 >2.3
UU Pegold Mira M 5.1 2.5 Ma90 14 <7.81 >0.7
WX Psc Mira M 36.9 18.1 Ma90 14 <0.21 >175.7
IK Tau (NRT) Mira M 46.9 23.0 Ma90 14 <0.57 >82.3
IK Tau (VLA) <0.17 >275.9
VX And SRa C <0.8 <0.8 Ol93 20 <1.4 Ol93 30 <0.28 >2.9:
RW LMi SRa C 59.6 21.9 Ma90 14 59.0 Ol93 20 75.8 Ol93 15 <0.96 >62.1
SS Vir SRa C <1.2 <1.2 Ol93 20 <1.72 >0.7
RT Cap SRb C 1.1 0.6 Ol88 15 <0.17 >6.5
CW Cnc SRb M 2.5 2.5 Ke99 20 <1.20 >2.1
RV Cyg SRb C 5.7 4.8 Ol87 20 16.7 Ol93 30 4.8 Ol93 20 <1.00 >5.7
V460 Cyg SRb C 4.7 4.7 Ol87 20 <1.53 >3.1
TU Gem SRb C 3.4 3.4 Ol93 20 <0.44 >7.7
T Mic SRb M 1.4 1.4 Ny92 20 <0.55 >2.5
Z Psc SRb C 0.9 1.0 Ol93 20 1.9 Ol93 30 <0.20 >4.5
R Scl SRb C 42.5 10.8 Kn85 7 27.0 Ol93 15 76.2 Ol93 30 <0.34 >125.0
U Ant Lb C 15.2 11.1 Ny92 20 10.8 Ol93 15 <2.64 >5.8
SZ Dra Lb M 0.8 0.8 Ke98 20 <0.77 >1.0
RAFGL 3068 ... C 56.3 6.9 Kn85 7 <0.98 >57.4
IRC-10529old (OH/IR) M 85.7 6.7 Kn85 7 14.3 Kn85 7 <4.95 >17.3
RAFGL 292 (LPVc) M 2.0 4.6 Da15 30 <0.25 >8.0
Confused NRT sources observed with the VLA
IRC +10216 (VLA) Mira C 395.0 123.1 Kn85 7 264.3 Ol93 20 310.7 Ol93 20 0.80 493.8
W HYa (VLA) SRa M 1.4 0.8 Ke99 15 <0.27 >5.2

Notes to the Table: For objects flagged as ‘old’ only less sensitive, non-digital H I spectra are available from our 1992/1993 observing campaign (see Sect. 2).

CO line flux references: Bu86 = Bujarrabal et al. (1986), Da15 = Danilovich et al. (2015), Di19 = Díaz-Luis et al. (2019),

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