MISCLASSIFIED
    MILKY WAY
 
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| LY Mus | IRAS 13372-7136 | GSC2.4.2 S7RV000162 | AAVSO 000-BDW-070 | 
| SIMBAD V* LY Mus | Pan-STARRS - | SAO 257077 | VSX 19949 | 
| GAIA DR3 5839896036299695104 | SkyMapper 134113.53-715205.4 | WRAY - | GCVS LY Mus | 
| 2MASS J13411359-7152056 | HIP 66783 | Hen 4-138 | BD - | 
| WISE J134113.50-715205.2 | TYC 9251-1340-1 | ESO - | HD 118685 | 
| Bidelman (1954) | - | Allen (1984) | - | Belzcyński et al. (2001) | - | 
| Gaposchkin (1957) | - | Kenyon (1986) | - | Akras et al. (2019) | - | 
| Boyarchuk (1969) | - | Vaidis (1988, 1991) | - | 
| Right ascension (°) | 205.3062Ref | Parallax (mas) | 3.250±0.051Ref | Reddening E(B-V) (mag) | 0.34±0.0Ref, Note | 
| Declination (°) | -71.8681Ref | Distance (kpc) | 0.31Ref, Note, 0.30Ref, Note | ||
| Galactic longitude (°) | 306.8300Ref | Proper motion in α (mas/yr) | -32.26±0.05Ref | ||
| Galactic latitude (°) | -9.3742Ref | Proper motion in δ (mas/yr) | 36.21±0.05Ref | 
Classified as a confirmed symbiotic binary in SIMBAD (Wenger et al., 2000) with the reference to Jorissen et al. (2012). The aforementioned article mentions weak Hα emission discovered by van Eck & Jorissen (2002). However, in van Eck & Jorissen (2002), the authors detected week Hα emission but claimed that it might be due to template mismatch.