POSSIBLE
MILKY WAY
|
| NSV 9601 | IRAS - | GSC2.4.2 S7Y2030106 | AAVSO - |
| SIMBAD NSV 9601 | Pan-STARRS 105432662832551050 | SAO - | VSX 48225 |
| GAIA DR3 4369320399740351872 | SkyMapper 174507.97-020828.0 | WRAY - | GCVS - |
| 2MASS J17450798-0208280 | HIP - | Hen - | BD - |
| WISE J174507.96-020827.7 | TYC - | ESO - | HD - |
| Bidelman (1954) | - | Allen (1984) | - | Belzcyński et al. (2001) | - |
| Gaposchkin (1957) | - | Kenyon (1986) | - | Akras et al. (2019) | - |
| Boyarchuk (1969) | - | Vaidis (1988, 1991) | NSV 9601 (incorrectly identified as HD 161224) (Susp.) |
| Right ascension (°) | 266.2833Ref | Parallax (mas) | 0.223±0.125Ref | Reddening E(B-V) (mag) | 0.36±0.02Ref, Note |
| Declination (°) | -2.1411Ref | Distance (kpc) | 5.28Ref, Note, 3.91Ref, Note | ||
| Galactic longitude (°) | 23.2591Ref | Proper motion in α (mas/yr) | -3.05±0.13Ref | ||
| Galactic latitude (°) | 13.6914Ref | Proper motion in δ (mas/yr) | -4.91±0.10Ref |
| X-Ray | - | IR type | S?Ref | Radio | - |
| X-Ray type | - | J (mag) | 15.94Ref | Flickering | - |
| GALEX FUV (mag) | - | H (mag) | 15.25Ref | Outbursts | - |
| GALEX NUV (mag) | - | K (mag) | 15.33Ref | Outburst type | - |
| IUE | NoRef | WISE W1 (mag) | 14.80Ref | Jets | - |
| FUSE | NoRef | WISE W2 (mag) | 14.87Ref | Resolved nebula | YesRef |
| U (mag) | - | WISE W3 (mag) | 11.97Ref | IPmax (eV) | 35.1Ref |
| B (mag) | - | WISE W4 (mag) | 8.42Ref | [O III] lines | YesRef |
| V (mag) | - | IRAS 12μm (Jy) | - | He II lines | - |
| R (mag) | - | IRAS 25μm (Jy) | - | [Fe VII] lines | - |
| I (mag) | - | IRAS 60μm (Jy) | - | O VI lines | - |
| BP (mag) | 18.55Ref | IRAS 100μm (Jy) | - | ||
| G (mag) | 17.83Ref | AKARI S09 (Jy) | - | ||
| RP (mag) | 17.00Ref | AKARI S18 (Jy) | - |
| Orbital period (days) | - | γ velocity (km/h) | - | Size of giant’s orbit (AU) | - |
| Eccentricity | - | RV of giant (km/h) | - | Separation (AU) | - |
| Inclination (°) | - | Inferior conj. of giant (JD) | - | Mass function | - |
| Eclipses | - | Mass ratio | - | ||
| Orbital ephemeris | - |
| Spectral type | - | Mass (M⊙) | - | Pulsation | - |
| Eff. temperature (K) | - | Radius (R⊙) | - | Type | - |
| IR type | S?Ref | Luminosity (L⊙) | - | Pulsation period (days) | - |
| Metallicity [Fe/H] | - | Pulsation ephemeris | - |
| Type/Spectral type | - | Mass (M⊙) | - | Spin period (min) | - |
| Shell-burning/Accreting-only | - | Radius (R⊙) | - | Accretion disk | - |
| Eff. temperature (K) | - | Luminosity (L⊙) | - | ||
| Lower limit (K) | - | ||||
| Upper limit (K) | - |
Suggested to be a symbiotic variable by Macconnell (1972), this star exhibits a probable detection of sharp Hα, Hβ, Hγ, and [O III] lines. The authors also reported the presence of a faint nebula associated with the object. This star is also listed in the catalog of Vaidis (1988).