POSSIBLE
MILKY WAY
|
| PTB 28 | IRAS 17374-1803 | GSC2.4.2 S808048912 | AAVSO - |
| SIMBAD Gaia DR3 4123293609265839488 | Pan-STARRS 86292650890586675 | SAO - | VSX 1541472 |
| GAIA DR3 4123293609265839488 | SkyMapper - | WRAY - | GCVS - |
| 2MASS J17402138-1805110 | HIP - | Hen - | BD - |
| WISE J174021.37-180511.1 | 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 (°) | 265.0891Ref | Parallax (mas) | -0.106±0.137Ref | Reddening E(B-V) (mag) | 0.41±0.01Ref, Note |
| Declination (°) | -18.0864Ref | Distance (kpc) | 7.49Ref, Note, 9.79Ref, Note | ||
| Galactic longitude (°) | 8.6393Ref | Proper motion in α (mas/yr) | -2.02±0.16Ref | ||
| Galactic latitude (°) | 6.6986Ref | Proper motion in δ (mas/yr) | -7.61±0.10Ref |
| X-Ray | - | IR type | D?Ref | Radio | - |
| X-Ray type | - | J (mag) | 9.69Ref | Flickering | - |
| GALEX FUV (mag) | - | H (mag) | 7.97Ref | Outbursts | - |
| GALEX NUV (mag) | - | K (mag) | 6.75Ref | Outburst type | - |
| IUE | NoRef | WISE W1 (mag) | 5.59Ref | Jets | - |
| FUSE | NoRef | WISE W2 (mag) | 4.52Ref | Resolved nebula | - |
| U (mag) | - | WISE W3 (mag) | 2.52Ref | IPmax (eV) | 35.1?Ref |
| B (mag) | - | WISE W4 (mag) | 1.24Ref | [O III] lines | YesRef |
| V (mag) | - | IRAS 12μm (Jy) | 4.71Ref | He II lines | - |
| R (mag) | - | IRAS 25μm (Jy) | 2.97Ref | [Fe VII] lines | - |
| I (mag) | - | IRAS 60μm (Jy) | 0.51Ref | O VI lines | - |
| BP (mag) | 18.38Ref | IRAS 100μm (Jy) | 4.32Ref | ||
| G (mag) | 15.21Ref | AKARI S09 (Jy) | 4.97Ref | ||
| RP (mag) | 13.65Ref | AKARI S18 (Jy) | 3.90Ref |
| 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 | YesRef |
| Eff. temperature (K) | - | Radius (R⊙) | - | Type | Mira?Ref |
| IR type | D?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) | - |
Classified as a symbiotic star candidate in the HASH Database of PNe (Parker et al., 2016), it was noted that the spectrum is PN-like, displaying Balmer lines, He I, [O III], [N II], and [S II] lines. However, the object is bright in 2MASS, z, and y PanSTARRS filters. Additionally, it might be a Mira variable according to VSX, and ZTF data supports Mira-like variability.