SUSPECTED
MILKY WAY
|
| PPA J1751-3103 | IRAS - | GSC2.4.2 S8DP015276 | AAVSO - |
| SIMBAD Gaia DR3 4055758753189074304 | Pan-STARRS - | SAO - | VSX - |
| GAIA DR3 4055758753189074304 | SkyMapper - | WRAY - | GCVS - |
| 2MASS J17510079-3103055 | HIP - | Hen - | BD - |
| WISE J175100.75-310305.8 | 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 (°) | 267.7532Ref | Parallax (mas) | -0.279±0.108Ref | Reddening E(B-V) (mag) | 1.86±0.11Ref, Note |
| Declination (°) | -31.0516Ref | Distance (kpc) | 9.51Ref, Note, 8.14Ref, Note | ||
| Galactic longitude (°) | 358.7901Ref | Proper motion in α (mas/yr) | -2.56±0.14Ref | ||
| Galactic latitude (°) | -2.0916Ref | Proper motion in δ (mas/yr) | -6.53±0.09Ref |
| X-Ray | NoRef | IR type | S?Ref | Radio | - |
| X-Ray type | - | J (mag) | 10.20Ref | Flickering | - |
| GALEX FUV (mag) | - | H (mag) | 8.91Ref | Outbursts | - |
| GALEX NUV (mag) | - | K (mag) | 8.08Ref | Outburst type | - |
| IUE | NoRef | WISE W1 (mag) | 6.87Ref | Jets | - |
| FUSE | NoRef | WISE W2 (mag) | 6.76Ref | Resolved nebula | - |
| U (mag) | - | WISE W3 (mag) | 5.71Ref | IPmax (eV) | 27.6Ref |
| B (mag) | - | WISE W4 (mag) | 4.61Ref | [O III] lines | NoRef |
| V (mag) | - | IRAS 12μm (Jy) | - | He II lines | NoRef |
| R (mag) | - | IRAS 25μm (Jy) | - | [Fe VII] lines | NoRef |
| I (mag) | - | IRAS 60μm (Jy) | - | O VI lines | NoRef |
| BP (mag) | 19.04Ref | IRAS 100μm (Jy) | - | ||
| G (mag) | 15.69Ref | AKARI S09 (Jy) | 0.31Ref | ||
| RP (mag) | 14.07Ref | 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 | shell-burning?Ref | Radius (R⊙) | - | Accretion disk | - |
| Eff. temperature (K) | - | Luminosity (L⊙) | - | ||
| Lower limit (K) | - | ||||
| Upper limit (K) | - |
Identified as a symbiotic star candidate in the HASH Database of PNe (Parker et al., 2016) based on the infrared colors suggestive of a symbiotic Mira. The spectrum displays a faint red continuum along with emission lines such as Balmer, [N II], and [S II]. The object's faintness in the WISE data introduces the possibility of alternative classifications, such as a compact H II region or a PN.