POSSIBLE
MILKY WAY
|
| OGLE-BLG-LPV-145820 | IRAS 17547-3343 | GSC2.4.2 S8GW404969 | AAVSO - |
| SIMBAD IRAS 17547-3343 | Pan-STARRS - | SAO - | VSX 303625 |
| GAIA DR3 4042384907898654080 | SkyMapper - | WRAY - | GCVS - |
| 2MASS J17580263-3344121 | HIP - | Hen - | BD - |
| WISE J175802.65-334412.0 | TYC - | ESO - | HD - |
| Bidelman (1954) | - | Allen (1984) | - | Belzcyński et al. (2001) | - |
| Gaposchkin (1957) | - | Kenyon (1986) | - | Akras et al. (2019) | - |
| Boyarchuk (1969) | - | Vaidis (1988, 1991) | - |
| Right ascension (°) | 269.5110Ref | Parallax (mas) | 0.256±0.344Ref | Reddening E(B-V) (mag) | 0.57±0.04Ref, Note |
| Declination (°) | -33.7367Ref | Distance (kpc) | 5.92Ref, Note, 6.21Ref, Note | ||
| Galactic longitude (°) | 357.2130Ref | Proper motion in α (mas/yr) | -0.55±0.37Ref | ||
| Galactic latitude (°) | -4.7249Ref | Proper motion in δ (mas/yr) | -4.01±0.26Ref |
| X-Ray | NoRef | IR type | D?Ref | Radio | - |
| X-Ray type | - | J (mag) | 12.86Ref | Flickering | - |
| GALEX FUV (mag) | - | H (mag) | 10.46Ref | Outbursts | - |
| GALEX NUV (mag) | - | K (mag) | 8.57Ref | Outburst type | - |
| IUE | NoRef | WISE W1 (mag) | 6.27Ref | Jets | - |
| FUSE | NoRef | WISE W2 (mag) | 4.48Ref | Resolved nebula | - |
| U (mag) | - | WISE W3 (mag) | 2.93Ref | IPmax (eV) | 13.6Ref |
| B (mag) | - | WISE W4 (mag) | 2.06Ref | [O III] lines | NoRef |
| V (mag) | 20.34Ref | IRAS 12μm (Jy) | 3.62Ref | He II lines | NoRef |
| R (mag) | - | IRAS 25μm (Jy) | 1.68Ref | [Fe VII] lines | NoRef |
| I (mag) | 16.40Ref | IRAS 60μm (Jy) | 1.21Ref | O VI lines | NoRef |
| BP (mag) | 19.57Ref | IRAS 100μm (Jy) | 28.20Ref | ||
| G (mag) | 18.63Ref | AKARI S09 (Jy) | 2.92Ref | ||
| RP (mag) | 16.40Ref | AKARI S18 (Jy) | 1.44Ref |
| 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 | CRef | Mass (M⊙) | - | Pulsation | YesRef |
| Eff. temperature (K) | - | Radius (R⊙) | - | Type | MiraRef |
| IR type | D?Ref | Luminosity (L⊙) | - | Pulsation period (days) | 600.5Ref |
| Metallicity [Fe/H] | - | Pulsation ephemeris | - |
| Type/Spectral type | - | Mass (M⊙) | - | Spin period (min) | - |
| Shell-burning/Accreting-only | shell-burning?Ref | Radius (R⊙) | - | Accretion disk | - |
| Eff. temperature (K) | - | Luminosity (L⊙) | - | ||
| Lower limit (K) | - | ||||
| Upper limit (K) | - |
The object is identified as a carbon-rich Mira, with a potential symbiotic nature inferred from the spectrum, according to observations in Matsunaga et al. (2017). The spectrum reveals the presence of low-excitation emission lines.