SUSPECTED
MILKY WAY
|
| ASAS J073507+1137.6 | IRAS - | GSC2.4.2 N8LS061032 | AAVSO 000-BGK-780 |
| SIMBAD ASAS J073507+1137.6 | Pan-STARRS 121951137775562747 | SAO - | VSX 83988 |
| GAIA DR3 3162213622082557184 | SkyMapper - | WRAY - | GCVS - |
| 2MASS J07350641+1137375 | HIP - | Hen - | BD - |
| WISE J073506.41+113737.5 | 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 (°) | 113.7771Ref | Parallax (mas) | 1.121±0.659Ref | Reddening E(B-V) (mag) | 0.02±0.0Ref, Note |
| Declination (°) | 11.6257Ref | Distance (kpc) | 1.25Ref, Note, 0.66Ref, Note | ||
| Galactic longitude (°) | 207.3049Ref | Proper motion in α (mas/yr) | 0.32±0.54Ref | ||
| Galactic latitude (°) | 14.8927Ref | Proper motion in δ (mas/yr) | -0.70±0.37Ref |
| X-Ray | - | IR type | - | Radio | - |
| X-Ray type | - | J (mag) | 7.84Ref | Flickering | - |
| GALEX FUV (mag) | 20.90Ref | H (mag) | 6.92Ref | Outbursts | - |
| GALEX NUV (mag) | 20.31Ref | K (mag) | 6.59Ref | Outburst type | - |
| IUE | NoRef | WISE W1 (mag) | 6.45Ref | Jets | - |
| FUSE | NoRef | WISE W2 (mag) | 6.43Ref | Resolved nebula | - |
| U (mag) | - | WISE W3 (mag) | 5.99Ref | IPmax (eV) | - |
| B (mag) | - | WISE W4 (mag) | 5.52Ref | [O III] lines | - |
| 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) | 19.53Ref | IRAS 100μm (Jy) | - | ||
| G (mag) | 19.63Ref | AKARI S09 (Jy) | 0.22Ref | ||
| RP (mag) | 16.81Ref | 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 | Yes?Ref |
| Eff. temperature (K) | - | Radius (R⊙) | - | Type | SR?Ref |
| IR type | - | Luminosity (L⊙) | - | Pulsation period (days) | 341.2399891Ref |
| Metallicity [Fe/H] | - | Pulsation ephemeris | - |
| Type/Spectral type | WDRef | Mass (M⊙) | - | Spin period (min) | - |
| Shell-burning/Accreting-only | - | Radius (R⊙) | - | Accretion disk | - |
| Eff. temperature (K) | - | Luminosity (L⊙) | - | ||
| Lower limit (K) | - | ||||
| Upper limit (K) | - |
Suspected of having a symbiotic nature by Akras (2023). The authors employed a combination of GALEX UV photometry, 2MASS/WISE IR photometry, and the ASAS-SN variables catalog to select the candidates.