Table 1
Properties of the suspected binaries in the MESS sample.
Object | Morphology | Spec. Type | d | Ṁ | vw | vLSR | Binary detection | References | |
[pc] | [10-7M⊙ yr-1] | [km s-1] | [km s-1] | ||||||
|
|||||||||
o Cet | Fermata and Irregular | M7 IIIe | 91 ± 10 | 2.5 | 8.1 | 107.7 | visual: ![]() |
(1),(2),(3) | |
θ Aps | Fermata | M6.5 III | 113 ± 6 | 1.1 | 4.5 | 34.2 | Hipparcos variability-induced mover (VIM) | (1),(2),(4),(5) | |
EP Aqr | Fermata | M8 IIIv | 114 ± 8 | 3.1 | 11.5 | 40.2 | complex CO profile | (1),(2),(6),(7) | |
π1 Gru | Irregular | S6e | 163 ± 20 | 8.5 | 30.0 | 11.9 | jets, visual: ![]() |
(1),(2),(8) | |
o1 Ori | Irregular | M3 | 200 ± 28 | < 0.4 | – | 38.8 | UV excess | (9),(10),(11) | |
R Aqr | Irregular | M7 IIIpev | 214 | 0.6 | 16.7 | 39.7 | symbiotic | (12),(13),(14),(15),(16),(17) | |
Y Lyn | Point source | M6 SIb-II | 253 ± 61 | 5.6 | 5.4 | 13.9 | Hipparcos VIM | (1),(9),(5) | |
TW Hor | Point source | C | 322 ± 38 | 0.24 | 7.5 | 52.4 | UV excess | (1),(18),(19),(16) | |
W Aql | Fermata | S6.6 | 340 | 130 | 20.0 | 21.6 | composite spectrum/CO profile, | (20),(2),(1),(21),(18),(22) | |
visual: ![]() |
|||||||||
R Scl | Fermata and Ring | C | 370 | 16 | 17.0 | 66.3 | spiral arm | (2),(1)(23) | |
VY UMa | Eye | C | 380 ± 51 | 0.7 | 7.9 | 28.2 | UV excess | (1),(4),(24),(10) | |
TX Cam | Point source | M8.5 | 380 | 65 | 21.2 | – | spiral arm | (2),(19) | |
U Cam | Eye | C | 430 | 10 | 20.6 | 9.8 | Hipparcos DMSA/C: ![]() |
(25),(26),(27),(1) | |
V Eri | Point source | M5/M6 IV | 439 ± 133 | 1.5 | 13 | 39.8 | UV excess | (1),(26),(24),(10) | |
RW LMi | Point source | C | 440 | 59 | 20.8 | – | spiral arm | (6),(2),(28) | |
VY CMa | Point source | M3/M4 III | 562 | 2800 | 46.5 | 42.9 | UV excess | (26),(2),(1),(10) | |
V Hya | Point source | C | 600 | 610 | 30 | 27.9 | rapid rotation | (14),(2),(1),(29) | |
LL Peg | Point source | C | 980 | 310 | 16.0 | – | spiral arm, visual: ![]() |
(2),(30),(31) | |
|
|||||||||
R Dor | Point source | M8 IIIe | 55 ± 3 | 6.1 | 6.0 | 39.4 | visual: ![]() |
(32),(33),(34) | |
W Hya | Ring | C | 104 ± 12 | 0.78 | 7.5 | 48.2 | visual: ![]() |
(1),(2),(34) | |
R Hya | Fermata | M7 IIIe | 124 ± 11 | 1.6 | 12.5 | 25.3 | visual: ![]() |
(1),(2),(34) | |
R Cas | Fermata | M7 IIIe | 127 ± 16 | 4.0 | 13.5 | 44.0 | visual: ![]() |
(1),(2),(34) | |
R Crt | Eye | M7 III | 261 ± 65 | 6.9 | 10.8 | 23.8 | visual: ![]() |
(1),(2),(34) | |
VX Sgr | Point source | M5/M6 III | 262 ± 187 | 610 | 24.3 | 8.5 | visual: ![]() |
(1),(2),(34) | |
UU Aur | Fermata | C | 341 | 2.7 | 11.0 | 17.9 | visual: ![]() |
(32),(2),(34) | |
V Pav | Eye | C | 370 ± 73 | 3.4 | 16.0 | 24.0 | visual: ![]() |
(1),(14),(24),(34) | |
S Sct | Ring | C | 386 ± 85 | 1.4 | 8.0 | 17.5 | visual: ![]() |
(1),(2),(34) | |
TT Cyg | Ring | C | 436 | 50 | 12.6 | 38.3 | visual: ![]() |
(32),(35),(36),(34) |
Notes. The table is subdivided into two parts. The upper part lists the physical binaries, the lower part the visual binaries without indicating physical association. The space motion vLSR is calculated following Johnson & Soderblom (1987). The adopted solar motion to convert heliocentric motion into LSR motion is (U,V,W)⊙ = (11.10,12.24,7.25) km s-1 (Schönrich et al. 2010). The objects are ordered by increasing distance. Although VX Sgr is associated with entry ADS 11078 in Proust et al. (1981), the Washington Double Star Catalog (http://ad.usno.navy.mil/wds/wdstext.html) does not list any measurement for that system, which is thus most likely spurious.
References. (1): van Leeuwen (2007), (2): De Beck et al. (2010), (3): Karovska et al. (1997), (4): Schöier & Olofsson (2001), (5): Pourbaix et al. (2003), (6): Knapp et al. (1998), (7): Winters et al. (2007), (8): Sahai (1992), (9): Groenewegen & de Jong (1998), (10): Sahai et al. (2008), (11): Ake & Johnson (1988), (12): Kamohara et al. (2010), (13): Matthews & Reid (2007), (14): Groenewegen et al. (2002), (15): Willson et al. (1981), (16): Hinkle et al. (1989), (17): Gromadzki & Mikołajewska (2009), (18): Culver et al. (1974), (19): Castro-Carrizo et al. (2010), (20): Guandalini & Busso (2008), (21): Herbig (1965), (22): Ramstedt et al. (2011), (23): Maercker et al. (2012), (24): Loup et al. (1993), (25): Knapp et al. (2003), (26): Young et al. (1993), (27): Lindqvist et al. (1999), (28): Dinh-V.-Trung & Lim (2009), (29): Barnbaum et al. (1995), (30): Mauron & Huggins (2006), (31): Morris et al. (2006), (32): Cox et al. (2012), (33): Olofsson et al. (2002), (34): Proust et al. (1981), (35): Olofsson (1996), (36): Olofsson et al. (2000)
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