Table 5: Galactic samples of red giants (Jura & Kleinmann 1989, 1990, 1992), with the spectral type, the stellar effective temperature, $T_{\rm eff}$ , the bolometric luminosity, L, and the mass-loss rates as determined by Jura & Kleinmann, $\dot{M}_1$ , and as predicted by our recipe, $\dot{M}_2$ . We omitted the IRAS prefix to some of the dust-enshrouded AGB stars.
Object Spectral $T_{\rm eff}$ $\log L$ $\log \dot{M}_1$ $\log \dot{M}_2$

type K $L_\odot$ $M_\odot$ /yr $M_\odot$ /yr

Intermediate-period AGB stars (Jura & Kleinmann 1992)

S CrB M 7 3126 3.70 -6.96 -5.66

R Leo M 8 2890 3.70 -7.07 -5.44

R LMi M 7 3126 3.70 -6.82 -5.66

RX Boo M 7.5 3008 3.70 -6.80 -5.55

W Hya M 7 3126 3.70 -7.00 -5.66

Dust-enshrouded AGB stars (Jura & Kleinmann 1989)

KU And M 9 2667 4.00 -4.72 -4.91

WX Psc M 9 2667 4.00 -4.64 -4.91

02316+6455 M 9 2667 4.00 -5.07 -4.91

02351-2711 M 9 2667 4.00 -5.44 -4.91

NML Tau M 6 3309 4.00 -5.22 -5.50

04307+6210 M 6 3309 4.00 -5.44 -5.50

TX Cam M 8.5 2778 4.00 -5.60 -5.02

05411+6957 M 9 2667 4.00 -5.23 -4.91

V Cam M 7 3126 4.00 -5.66 -5.34

06300+6058 M 9 2667 4.00 -5.28 -4.91

GX Mon M 9 2667 4.00 -5.03 -4.91

IW Hya M 9 2667 4.00 -5.02 -4.91

V2108 Oph M 9 2667 4.00 -5.42 -4.91

V774 Sgr M 5 3434 4.00 -5.55 -5.60

18009-2019 M 8 2890 4.00 -5.37 -5.12

18135-1641 M 5 3434 4.00 -5.30 -5.60

18204-1344 M 8 2890 4.00 -5.38 -5.12

V1111 Oph M 9 2667 4.00 -5.28 -4.91

18413+1354 M 7 3126 4.00 -5.26 -5.34

V3953 Sgr M 9 2667 4.00 -5.17 -4.91

V3880 Sgr M 8 2890 4.00 -5.00 -5.12

V342 Sgr M 9 2667 4.00 -5.36 -4.91

20440-0105 M 9 2667 4.00 -5.57 -4.91

UU Peg M 7 3126 4.00 -5.80 -5.34

RT Cep M 6 3309 4.00 -5.60 -5.50

23496+6131 M 9 2667 4.00 -5.27 -4.91

Red supergiants (Jura & Kleinmann 1990)

KW Sgr M 0Ia 3895 5.00 -5.40 -4.89

VX Sgr M 4Ia 3574 5.18 -4.40 -4.47

UY Sct M 4Iab 3574 5.00 -5.15 -4.66

BD+24 $^\circ$ 3902 M 1Ia 3810 5.00 -6.00 -4.83

BI Cyg M 4Ia 3574 5.30 -5.22 -4.34

KY Cyg M 3.5Ia 3620 5.60 -5.40 -4.06

NML Cyg M 6III 3309 5.70 -4.00 -3.71

$\mu$ Cep M 2Ia 3736 5.60 -6.05 -4.15

PZ Cas M 2Ia 3736 5.30 -5.00 -4.46

TZ Cas M 2Iab 3736 5.00 -5.52 -4.78

S Per M 3Ia 3666 5.30 -5.15 -4.41

SU Per M 3Iab 3666 5.00 -5.22 -4.73

$\alpha$ Ori M 1 3810 5.00 -6.70 -4.83

VY CMa M 5I 3434 5.60 -4.00 -3.92

EV Car M 4Ia 3574 5.30 -5.22 -4.34

CK Car M 3.5Iab 3620 5.00 -5.70 -4.69

IX Car M 2Iab 3736 5.00 -5.05 -4.78

V396 Cen M 4Ia 3574 5.30 -6.00 -4.34

AH Sco M 4 3574 5.48 -5.10 -4.16

**Table 5:** Galactic samples of red giants (Jura & Kleinmann 1989, 1990, 1992), with the spectral type, the stellar effective temperature, $T_{\rm eff}$ , the bolometric luminosity, L, and the mass-loss rates as determined by Jura & Kleinmann, $\dot{M}_1$ , and as predicted by our recipe, $\dot{M}_2$ . We omitted the IRAS prefix to some of the dust-enshrouded AGB stars.
Object	Spectral	$T_{\rm eff}$	$\log L$	$\log \dot{M}_1$	$\log \dot{M}_2$
	type	K	$L_\odot$	$M_\odot$ /yr	$M_\odot$ /yr
Intermediate-period AGB stars (Jura & Kleinmann 1992)
S CrB	M 7	3126	3.70	-6.96	-5.66
R Leo	M 8	2890	3.70	-7.07	-5.44
R LMi	M 7	3126	3.70	-6.82	-5.66
RX Boo	M 7.5	3008	3.70	-6.80	-5.55
W Hya	M 7	3126	3.70	-7.00	-5.66
Dust-enshrouded AGB stars (Jura & Kleinmann 1989)
KU And	M 9	2667	4.00	-4.72	-4.91
WX Psc	M 9	2667	4.00	-4.64	-4.91
02316+6455	M 9	2667	4.00	-5.07	-4.91
02351-2711	M 9	2667	4.00	-5.44	-4.91
NML Tau	M 6	3309	4.00	-5.22	-5.50
04307+6210	M 6	3309	4.00	-5.44	-5.50
TX Cam	M 8.5	2778	4.00	-5.60	-5.02
05411+6957	M 9	2667	4.00	-5.23	-4.91
V Cam	M 7	3126	4.00	-5.66	-5.34
06300+6058	M 9	2667	4.00	-5.28	-4.91
GX Mon	M 9	2667	4.00	-5.03	-4.91
IW Hya	M 9	2667	4.00	-5.02	-4.91
V2108 Oph	M 9	2667	4.00	-5.42	-4.91
V774 Sgr	M 5	3434	4.00	-5.55	-5.60
18009-2019	M 8	2890	4.00	-5.37	-5.12
18135-1641	M 5	3434	4.00	-5.30	-5.60
18204-1344	M 8	2890	4.00	-5.38	-5.12
V1111 Oph	M 9	2667	4.00	-5.28	-4.91
18413+1354	M 7	3126	4.00	-5.26	-5.34
V3953 Sgr	M 9	2667	4.00	-5.17	-4.91
V3880 Sgr	M 8	2890	4.00	-5.00	-5.12
V342 Sgr	M 9	2667	4.00	-5.36	-4.91
20440-0105	M 9	2667	4.00	-5.57	-4.91
UU Peg	M 7	3126	4.00	-5.80	-5.34
RT Cep	M 6	3309	4.00	-5.60	-5.50
23496+6131	M 9	2667	4.00	-5.27	-4.91
Red supergiants (Jura & Kleinmann 1990)
KW Sgr	M 0Ia	3895	5.00	-5.40	-4.89
VX Sgr	M 4Ia	3574	5.18	-4.40	-4.47
UY Sct	M 4Iab	3574	5.00	-5.15	-4.66
BD+24 $^\circ$ 3902	M 1Ia	3810	5.00	-6.00	-4.83
BI Cyg	M 4Ia	3574	5.30	-5.22	-4.34
KY Cyg	M 3.5Ia	3620	5.60	-5.40	-4.06
NML Cyg	M 6III	3309	5.70	-4.00	-3.71
$\mu$ Cep	M 2Ia	3736	5.60	-6.05	-4.15
PZ Cas	M 2Ia	3736	5.30	-5.00	-4.46
TZ Cas	M 2Iab	3736	5.00	-5.52	-4.78
S Per	M 3Ia	3666	5.30	-5.15	-4.41
SU Per	M 3Iab	3666	5.00	-5.22	-4.73
$\alpha$ Ori	M 1	3810	5.00	-6.70	-4.83
VY CMa	M 5I	3434	5.60	-4.00	-3.92
EV Car	M 4Ia	3574	5.30	-5.22	-4.34
CK Car	M 3.5Iab	3620	5.00	-5.70	-4.69
IX Car	M 2Iab	3736	5.00	-5.05	-4.78
V396 Cen	M 4Ia	3574	5.30	-6.00	-4.34
AH Sco	M 4	3574	5.48	-5.10	-4.16

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observational data
	3 Analysis
	4 Mass-loss rate as a function of bolometric luminosity and stellar effective temperature
	5 The Hertzsprung-Russell diagram of dust-enshrouded AGB stars and red supergiants
	6 Summary
	Appendix A: Spectra of galactic M-type stars
	References