CONFIRMED
MILKY WAY
|
| [MMU2013] 354.98-02.87 | IRAS 17415-3441 | GSC2.4.2 S8BA043037 | AAVSO - |
| SIMBAD IRAS 17415-3441 | Pan-STARRS - | SAO - | VSX 305978 |
| GAIA DR3 4041342811385576704 | SkyMapper - | WRAY - | GCVS - |
| 2MASS J17445312-3442395 | HIP - | Hen - | BD - |
| WISE J174453.12-344239.7 | TYC - | ESO - | HD - |
| Bidelman (1954) | - | Allen (1984) | - | Belzcyński et al. (2001) | - |
| Gaposchkin (1957) | - | Kenyon (1986) | - | Akras et al. (2019) | 354.98-02.87 (Conf.) |
| Boyarchuk (1969) | - | Vaidis (1988, 1991) | - |
| Right ascension (°) | 266.2213Ref | Parallax (mas) | 0.145±0.136Ref | Reddening E(B-V) (mag) | 0.9±0.02Ref, Note |
| Declination (°) | -34.7111Ref | Distance (kpc) | 5.99Ref, Note, 4.84Ref, Note | ||
| Galactic longitude (°) | 354.9878Ref | Proper motion in α (mas/yr) | -0.73±0.17Ref | ||
| Galactic latitude (°) | -2.8762Ref | Proper motion in δ (mas/yr) | -7.70±0.09Ref |
| X-Ray | - | IR type | D?Ref | Radio | - |
| X-Ray type | - | J (mag) | 14.55Ref | Flickering | - |
| GALEX FUV (mag) | - | H (mag) | 12.57Ref | Outbursts | - |
| GALEX NUV (mag) | - | K (mag) | 10.75Ref | Outburst type | - |
| IUE | NoRef | WISE W1 (mag) | 8.01Ref | Jets | - |
| FUSE | NoRef | WISE W2 (mag) | 6.58Ref | Resolved nebula | - |
| U (mag) | - | WISE W3 (mag) | 3.95Ref | IPmax (eV) | 114Ref |
| B (mag) | - | WISE W4 (mag) | 2.25Ref | [O III] lines | YesRef |
| V (mag) | - | IRAS 12μm (Jy) | 2.13Ref | He II lines | YesRef |
| R (mag) | - | IRAS 25μm (Jy) | 1.31Ref | [Fe VII] lines | NoRef |
| I (mag) | - | IRAS 60μm (Jy) | 0.99Ref | O VI lines | YesRef |
| BP (mag) | 17.92Ref | IRAS 100μm (Jy) | 10.00Ref | ||
| G (mag) | 17.59Ref | AKARI S09 (Jy) | - | ||
| RP (mag) | 16.70Ref | AKARI S18 (Jy) | 1.06Ref |
| 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-burningRef | Radius (R⊙) | - | Accretion disk | - |
| Eff. temperature (K) | - | Luminosity (L⊙) | - | ||
| Lower limit (K) | 114000Ref | ||||
| Upper limit (K) | - |
This object displays a typical D-type emission-line spectrum, including a weak detection of the Raman-scattered O VI 6825 feature. The very red 2MASS colors align well with the known symbiotic Miras, as mentioned in Miszalski et al. (2013).