IRAS 19558+3333
POSSIBLE
MILKY WAY
Constellation
Cygnus |
Equatorial coordinates
α = 19 57 48.449
δ = +33 41 21.250 |
Galactic coordinates
l = 69.9830°
b = 2.3764° |
| Suspected |
1994Ref |
| Confirmed |
- |
| Symbiotic IR type |
D?Ref |
| Hot component type |
shell-burning?Ref |
| Outbursts |
- |
|
|
Symbiotic Catalogs
| Bidelman (1954) |
- |
Allen (1984) |
- |
Belzcyński et al. (2001) |
IRAS 19558+3333 (Susp.) |
| Gaposchkin (1957) |
- |
Kenyon (1986) |
- |
Akras et al. (2019) |
IRAS 19558+3333 (Susp.) |
| Boyarchuk (1969) |
- |
Vaidis (1988, 1991) |
- |
Position
| Right ascension (°) |
299.4519Ref |
Parallax (mas) |
- |
Reddening E(B-V) (mag) |
0.69±0.01Ref, Note |
| Declination (°) |
33.6892Ref |
Distance (kpc) |
-, Note |
|
|
| Galactic longitude (°) |
69.9830Ref |
Proper motion in α (mas/yr) |
- |
|
|
| Galactic latitude (°) |
2.3764Ref |
Proper motion in δ (mas/yr) |
- |
|
|
Observations
| X-Ray |
- |
IR type |
D?Ref |
Radio |
YesRef |
| X-Ray type |
- |
J (mag) |
17.90Ref |
Flickering |
- |
| GALEX FUV (mag) |
- |
H (mag) |
15.51Ref |
Outbursts |
- |
| GALEX NUV (mag) |
- |
K (mag) |
11.62Ref |
Outburst type |
- |
| IUE |
NoRef |
WISE W1 (mag) |
6.50Ref |
Jets |
- |
| FUSE |
NoRef |
WISE W2 (mag) |
3.41Ref |
Resolved nebula |
- |
| U (mag) |
- |
WISE W3 (mag) |
0.06Ref |
IPmax (eV) |
- |
| B (mag) |
- |
WISE W4 (mag) |
-1.32Ref |
[O III] lines |
- |
| V (mag) |
- |
IRAS 12μm (Jy) |
42.90Ref |
He II lines |
- |
| R (mag) |
- |
IRAS 25μm (Jy) |
46.00Ref |
[Fe VII] lines |
- |
| I (mag) |
- |
IRAS 60μm (Jy) |
12.50Ref |
O VI lines |
- |
| BP (mag) |
- |
IRAS 100μm (Jy) |
38.40Ref |
|
|
| G (mag) |
- |
AKARI S09 (Jy) |
31.09Ref |
|
|
| RP (mag) |
- |
AKARI S18 (Jy) |
26.87Ref |
|
|
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) |
- |
|
|
|
|
| Upper limit (K) |
- |
|
|
|
|
Notes
First identified as a potential symbiotic star in Seaquist & Ivison (1994). Later classified as an extreme D-type symbiotic system, with the presence of radio continuum emission suggesting the existence of a hot companion (Belczyński et al., 2000).
References
- Belczyński, K., Mikołajewska, J., Munari, U. et al., 2000, A&AS, 146, 407, 2000A&AS..146..407B
- Seaquist, E. R., Ivison, R. J., 1994, MNRAS, 269, 512, 1994MNRAS.269..512S
Last updated: August 21, 2021