Table 1.

Sample of oxygen stars

Name	R.A.	Decl.	VLSR	D	T ⋆	L ⋆	Ṁ	V exp	T d(rc)	r c	Ψ
	J2000.0	J2000.0	(km s−1)	(pc)	(K)	(L⊙)	(M⊙ yr−1)	(km s−1)	(K)	(cm)
IK Tau	03:53:28.87	+11:24:21.7	+34.5 e	285 a	2100 b	9250 b∗	2.4 × 10−5 b∗	17.5 e	1000 b	1.8 × 1014 b	435 i
KUAnd	00:06:52.94	+43:05:00.0	-22	680 c	2000 c	11800 c	9.4 × 10−6 d	19.5	1100 c	1.5 × 1014 c	200 m
RXBoo	14:24:11.63	+25:42:13.4	+1.5	128 a	1800 c	4550 c∗	6.1 × 10−7 b∗	7.5	900 c	1.5 × 1014 c	144 x
RT Vir	13:02:37.98	+05:11:08.4	+18.5	226 l	2000 b	4500 b	4.5 × 10−7 b	7	1000 b	1.6 × 1014 b	2000 q
RLeo	09:47:33.49	+11:25:43.7	+0.1	71 a	2000 b	2500 b	1.0 × 10−7 b	5	1200 b	1.3 × 1014 b	167 m
WXPsc	01:06:25.98	+12:35:53.1	+9.5	700 b	1800 b	10300 b	4.0 × 10−5 b	19	800 b	3.2 × 1014 b	250 m
GXMon	06:52:46.91	+08:25:19.0	-9.5	416 a	2600 c	4700 c∗	4.9 × 10−6 d∗	18	900 c	1.1 × 1014 c	200 m
NVAur	05:11:19.44	+52:52:33.2	+3	1200 c	2000 c	9800 c	2.5 × 10−5 d	17.5	1100 c	1.7 × 1014 c	1000 m
V1111Oph	18:37:19.26	+10:25:42.2	-31	357 a	1800 b	2300 b∗	2.7 × 10−6 d∗	15.5	800 b	2.7 × 1014 b	200 m
RRAql	19:57:36.06	-01:53:11.3	+28	318 a	2000 c	2800 c∗	8.6 × 10−7 d∗	8.5	1500 c	5.9 × 1013 c	185 t
RLMi	09:45:34.28	+34:30:42.8	+0.9	330 d	2400 d	5500 d	2.6 × 10−7 d	5.5	1000 d	1.7 × 1014 d	115 t
BXCam	05:46:44.10	+69:58:25.2	-1	244 a	2800 c	1800 c∗	1.0 × 10−6 d∗	17	1500 c	7.1 × 1013 c	300 z
V1300 Aql	20:10:27.87	-06:16:13.6	-17.5	620 c	2000 c	10600 c	1.0 × 10−5 d	15	1100 c	1.8 × 1014 c	1000 m
RCas	23:58:24.87	+51:23:19.7	+26.5	188 a	1800 e	10400 e∗	9.5 × 10−7 e∗	7.5	1050 e	2.5 × 1014 e	91 m
IRC -30398	18:59:13.85	-29:50:20.4	-7.5	390 m	2000 m	8700 m	6.0 × 10−6 m	14.5	800 b	2.6 × 1014 b	200 m
TXCam	05:00:50.40	+56:10:52.6	+11.5	334 a	2600 c	6600 c∗	7.7 × 10−6 c∗	17.5	1300 c	1.0 × 1014 c	500 x
SCrB	15:21:23.96	+31:22:02.6	+1.5	431 a	2400 d	6300 d∗	2.7 × 10−7 d∗	5	1000 d	1.7 × 1014 d	300 z
IRC +60169	06:34:34.88	+60:56:33.2	-22	510 a	2200 c	5900 c∗	9.6 × 10−6 c∗	15	1000 c	1.1 × 1014 c	300 z
RHya	13:29:42.78	-23:16:52.8	-10 o	224 a	2600 c	17200 c∗	4.7 × 10−7 c∗	5 o	1500 c	6.1 × 1013 c	200 m
R Crt	11:00:33.85	-18:19:29.6	+11.5	236 a	2800 c	7700 c∗	1.0 × 10−6 c∗	11	600 c	3.5 × 1014 c	333 q
o Ceti	02:19:20.79	-02:58:39.5	+47	107 f	3000 g	9000 g	2.0 × 10−7 h	3	1000 z	9.7 × 1013 y	195 t
WHya	13:49:02.00	-28:22:03.5	+40.5	164 a	2600 b	16800 b∗	4.2 × 10−7 b∗	6	1200 b	6.3 × 1013 b	500 v
TCep	21:09:31.78	+68:29:27.2	-2.5	176 a	2400 d	4900 d∗	7.8 × 10−8 d∗	4	1000 d	1.8 × 1014 d	300 z
V1943 Sgr	20:06:55.24	-27:13:29.8	-14.5	666 a	2200 d	55400 d∗	1.0 × 10−6 d∗	4.5	1000 d	1.6 × 1014 d	300 z
SW Vir	13:14:04.39	-02:48:25.2	-10.5	300 a	2400 b	17600 b∗	2.2 × 10−6 b∗	7.5	800 b	2.9 × 1014 b	1000 q
AFGL292	02:02:38.63	+07:40:36.5	+23.7	253 a	2200 d	6000 d	1.3 × 10−7 d∗	7	1000 d	1.8 × 1014 d	300 z
BK Vir	12:30:21.01	+04:24:59.2	+17.5	234 a	3000 n	4500 n∗	2.3 × 10−7 m∗	4	1000 z	8.6 × 1013 z	2000 q

References and notes: The coordinates of the O-rich stars are taken from the literature. An asterisk in the value of the luminosity (L_⋆) or mass loss rate (M) indicates that the value has been scaled according to the updated value of the distance.

^a Gaia Collaboration et al. (2018),

^b Ramstedt & Olofsson (2014),

^c Schöier et al. (2013),

^d Danilovich et al. (2015),

^e Maercker et al. (2016),

^f Knapp et al. (2003),

^g Woodruff et al. (2004),

^h Ryde & Schöier (2001),

ⁱ Gobrecht et al. (2016),

^k Justtanont et al. (1996),

^l Zhang et al. (2017),

^m González Delgado et al. (2003),

ⁿ Ohnaka et al. (2011),

^o Knapp et al. (1998),

^p De Beck et al. (2010),

^q Olofsson et al. (2002),

^r Dyck et al. (1996),

^s Winters et al. (2007),

^t Groenewegen et al. (1999),

^v Khouri et al. (2014),

^x Dharmawardena et al. (2018),

^w Gardan et al. (2006),

^y Kamiński et al. (2016)

^zAssumed value for the condensation radius r_c is 5 R_⋆, for the dust temperature at the condensation radius Td(r_c) is 1000 K, and for the gas-to-dust mass ratio Ψ is 300.