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