SUSPECTED
MILKY WAY
|
| ASASSN-17dm | IRAS 10048-4728 | GSC2.4.2 S5N8000332 | AAVSO 000-BMG-387 |
| SIMBAD ASASSN -17dm | Pan-STARRS - | SAO - | VSX 477461 |
| GAIA DR3 5407536006622793984 | SkyMapper 100657.55-474341.7 | WRAY - | GCVS - |
| 2MASS J10065752-4743419 | HIP - | Hen - | BD - |
| WISE J100657.53-474341.8 | 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 (°) | 151.7397Ref | Parallax (mas) | 0.258±0.020Ref | Reddening E(B-V) (mag) | 0.16±0.01Ref, Note |
| Declination (°) | -47.7283Ref | Distance (kpc) | 3.79Ref, Note, 4.38Ref, Note | ||
| Galactic longitude (°) | 276.4934Ref | Proper motion in α (mas/yr) | -7.29±0.02Ref | ||
| Galactic latitude (°) | 6.5212Ref | Proper motion in δ (mas/yr) | 4.15±0.02Ref |
| X-Ray | - | IR type | D?Ref | Radio | - |
| X-Ray type | - | J (mag) | 9.15Ref | Flickering | - |
| GALEX FUV (mag) | - | H (mag) | 7.88Ref | Outbursts | YesRef |
| GALEX NUV (mag) | - | K (mag) | 6.92Ref | Outburst type | - |
| IUE | NoRef | WISE W1 (mag) | 5.26Ref | Jets | - |
| FUSE | NoRef | WISE W2 (mag) | 4.29Ref | Resolved nebula | Yes?Ref |
| U (mag) | - | WISE W3 (mag) | 2.62Ref | IPmax (eV) | - |
| B (mag) | 16.70Ref | WISE W4 (mag) | 1.46Ref | [O III] lines | - |
| V (mag) | 14.10Ref | IRAS 12μm (Jy) | 3.06Ref | He II lines | - |
| R (mag) | - | IRAS 25μm (Jy) | 2.27Ref | [Fe VII] lines | - |
| I (mag) | - | IRAS 60μm (Jy) | 2.49Ref | O VI lines | - |
| BP (mag) | 14.53Ref | IRAS 100μm (Jy) | 3.94Ref | ||
| G (mag) | 12.71Ref | AKARI S09 (Jy) | 3.00Ref | ||
| RP (mag) | 11.41Ref | AKARI S18 (Jy) | 2.25Ref |
| Orbital period (days) | - | γ velocity (km/h) | 43.16±0.25Ref | 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 | MRef | 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 | - | Radius (R⊙) | - | Accretion disk | - |
| Eff. temperature (K) | - | Luminosity (L⊙) | - | ||
| Lower limit (K) | - | ||||
| Upper limit (K) | - |
Suggested to be a probable supernova in AKARI J1006572-474345 (Kiyota et al., 2017), further investigations revealed a spectrum resembling a foreground M-type star, possibly a nova or symbiotic star in outburst (Fraser et al., 2017). They asserted that the extended source is not a galaxy but a potential nebula. Subsequent confirmation of the M-type spectrum was reported (Morrell et al., 2017). The object is classified as a confirmed symbiotic star in the ASAS-SN database (Jayasinghe et al., 2019).