SUSPECTED
MILKY WAY
|
| MaC 1-10 | IRAS 18061-2505 | GSC2.4.2 S9SF099243 | AAVSO - |
| SIMBAD PN MaC 1-10 | Pan-STARRS 77902723017268790 | SAO - | VSX - |
| GAIA DR3 4065774303370565376 | SkyMapper 180912.42-250434.4 | WRAY - | GCVS - |
| 2MASS J18091242-2504344 | HIP - | Hen - | BD - |
| WISE J180912.41-250434.3 | 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 (°) | 272.3017Ref | Parallax (mas) | -0.545±0.436Ref | Reddening E(B-V) (mag) | 1.34±0.05Ref, Note |
| Declination (°) | -25.0763Ref | Distance (kpc) | 6.10Ref, Note, 3.14Ref, Note | ||
| Galactic longitude (°) | 5.9736Ref | Proper motion in α (mas/yr) | -0.22±0.51Ref | ||
| Galactic latitude (°) | -2.6112Ref | Proper motion in δ (mas/yr) | -8.64±0.36Ref |
| X-Ray | - | IR type | D'?Ref | Radio | YesRef |
| X-Ray type | - | J (mag) | 14.39Ref | Flickering | - |
| GALEX FUV (mag) | - | H (mag) | 12.81Ref | Outbursts | - |
| GALEX NUV (mag) | - | K (mag) | 10.89Ref | Outburst type | - |
| IUE | NoRef | WISE W1 (mag) | 8.31Ref | Jets | - |
| FUSE | NoRef | WISE W2 (mag) | 6.88Ref | Resolved nebula | YesRef |
| U (mag) | - | WISE W3 (mag) | 1.75Ref | IPmax (eV) | 35.1Ref |
| B (mag) | - | WISE W4 (mag) | -0.77Ref | [O III] lines | YesRef |
| V (mag) | - | IRAS 12μm (Jy) | 5.92Ref | He II lines | NoRef |
| R (mag) | - | IRAS 25μm (Jy) | 20.60Ref | [Fe VII] lines | NoRef |
| I (mag) | - | IRAS 60μm (Jy) | 22.60Ref | O VI lines | NoRef |
| BP (mag) | 16.96Ref | IRAS 100μm (Jy) | 165.00Ref | ||
| G (mag) | 16.96Ref | AKARI S09 (Jy) | 2.79Ref | ||
| RP (mag) | 15.17Ref | AKARI S18 (Jy) | 12.06Ref |
| 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 | 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 HASH Database of PNe (Parker et al., 2016). Exhibits highly collimated bipolar outflows. The spectrum displays Balmer lines, [O III], [S II], and [N II] in emission. Additionally suggested to be a PN with a WR central star (Górny et al., 2004).