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Table 1

Target properties and phenomenology.

Target name: R Aql R Aqr R Hya W Hya V Hya
HIP 93820 HIP 117054 HIP 65835 HIP 67419 HIP 53085
Associated calibratora: η Sgr, ϵ Peg 30 Psc 2 Cen 2 Cen α Hya

Type: Mira Mira Mira Mira/SRa SRa/L
Chemistry: O-rich O-rich O-rich O-rich C-rich
Massb (M): 1.0 1.5 2.0 1.0 1.0
Distancec (pc): 250 ±  50 130 ±  25 360 ±  70
12 μm fluxd (Jy): 402 ±  36 1580 ±  60 1590 ±  80 4200 ±  210 1110 ±  60
Spectral classificatione: M7 III e var M7 III pev M7 III e g M7 III e g N; C7, 5e
Effective temperatureb (K): 3000 ±  300 2800 ±  300 2700 ±  300 2500 ±  300 2650 ±  300
Luminosityb (L): 3470 ±  500 5000 ±  500 11 600 ±  1000 5400 ±  500 7850 ±  500
K-band diameterf (mas): 11.5 ±  1.4 16.6 ±  3.0 24.5 ±  1.2 42.8 ±  3.2 14.5 ±  0.3
Mass-loss rateg (10-7 M yr-1): 6–35 0.1–9 0.1–2 0.8–5 10–600
Multiplicityb: triple system SB wide binary wide binary wide binary
Evolutionary stageb: TP-AGB TP-AGB TP-AGB early-AGB post-AGB
Jets/fast windb: no yes no no yes
Asymmetryb: maybe yes no yes yes
Maserb: SiO, H2O, OH SiO, H2O, OH SiO, H2O, OH SiO, H2O, OH CO?
Periodb: decreasing stable decreasing stable two periods
Othersb: recent symbiotic detached common
He flash system shell, recent envelope,
(Mira+WD) He flash rapid rotator

Notes. 

(a)

For calibrator properties see Sect. 3.1 and Table 3.

(b)

See text for references, errors are approximations derived from the values found in the literature.

(c)

For R Aqr, R Hya and V Hya derived from the period-luminosity relation (cf.  Whitelock et al. 2008), and for R Aql and W Hya obtained from maser measurements (Kamohara et al. 2010; Vlemmings et al. 2003, respectively).

(d)

IRAS flux (Neugebauer et al. 1984).

(e)

SIMBAD.

(f)

Values are averages from the literature (cf. Sect. 4.4).

(g)

Range of current mass-loss rates as given in Sect. 2. For W Hya see e.g. De Beck et al. (2010), Muller et al. (2008) and Justtanont et al. (2005).

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