[MMU2013] 357.12+01.66
LIKELY
MILKY WAY
Constellation
Scorpius |
Equatorial coordinates
α = 17 32 04.767
δ = -30 28 54.758 |
Galactic coordinates
l = 357.1238°
b = 1.6618° |
| Suspected |
2013Ref |
| Confirmed |
- |
| Symbiotic IR type |
D?Ref |
| Hot component type |
shell-burning?Ref |
| Outbursts |
- |
|
|
Symbiotic Catalogs
| Bidelman (1954) |
- |
Allen (1984) |
- |
Belzcyński et al. (2001) |
- |
| Gaposchkin (1957) |
- |
Kenyon (1986) |
- |
Akras et al. (2019) |
357.12+01.66 (Susp.) |
| Boyarchuk (1969) |
- |
Vaidis (1988, 1991) |
- |
Position
| Right ascension (°) |
263.0199Ref |
Parallax (mas) |
-0.005±0.094Ref |
Reddening E(B-V) (mag) |
3.09±0.22Ref, Note |
| Declination (°) |
-30.4819Ref |
Distance (kpc) |
8.79Ref, Note, 6.38Ref, Note |
|
|
| Galactic longitude (°) |
357.1238Ref |
Proper motion in α (mas/yr) |
-3.29±0.09Ref |
|
|
| Galactic latitude (°) |
1.6618Ref |
Proper motion in δ (mas/yr) |
-5.93±0.07Ref |
|
|
Observations
| X-Ray |
NoRef |
IR type |
D?Ref |
Radio |
- |
| X-Ray type |
- |
J (mag) |
11.03Ref |
Flickering |
- |
| GALEX FUV (mag) |
- |
H (mag) |
9.01Ref |
Outbursts |
- |
| GALEX NUV (mag) |
- |
K (mag) |
7.46Ref |
Outburst type |
- |
| IUE |
NoRef |
WISE W1 (mag) |
5.52Ref |
Jets |
- |
| FUSE |
NoRef |
WISE W2 (mag) |
4.48Ref |
Resolved nebula |
- |
| U (mag) |
- |
WISE W3 (mag) |
2.97Ref |
IPmax (eV) |
13.6Ref |
| B (mag) |
- |
WISE W4 (mag) |
1.32Ref |
[O III] lines |
NoRef |
| V (mag) |
- |
IRAS 12μm (Jy) |
4.02Ref |
He II lines |
NoRef |
| R (mag) |
- |
IRAS 25μm (Jy) |
2.94Ref |
[Fe VII] lines |
NoRef |
| I (mag) |
- |
IRAS 60μm (Jy) |
2.61Ref |
O VI lines |
NoRef |
| BP (mag) |
17.78Ref |
IRAS 100μm (Jy) |
90.50Ref |
|
|
| G (mag) |
16.17Ref |
AKARI S09 (Jy) |
- |
|
|
| RP (mag) |
14.74Ref |
AKARI S18 (Jy) |
2.17Ref |
|
|
Orbit
| 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 |
- |
|
|
|
|
Cool component
| 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 |
- |
Hot component
| 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) |
14000Ref |
|
|
|
|
| Upper limit (K) |
- |
|
|
|
|
References
- Akras, S., Leal-Ferreira, M. L., Guzman-Ramirez, L. et al., 2019, MNRAS, 483, 4, 5077, 2019MNRAS.483.5077A
- Miszalski, B., Mikołajewska, J., Udalski, A., 2013, MNRAS, 432, 4, 3186, 2013MNRAS.432.3186M
Last updated: May 3, 2022