Wil 1 SySt-1
SUSPECTED
WILLMAN 1
Constellation
Ursa Major |
Equatorial coordinates
α = 10 49 27.858
δ = +51 03 46.160 |
Galactic coordinates
l = 158.5391°
b = 56.7877° |
Suspected |
2020Ref |
Confirmed |
- |
Symbiotic IR type |
- |
Hot component type |
- |
Outbursts |
- |
|
|
Symbiotic Catalogs
Bidelman (1954) |
- |
Allen (1984) |
- |
Belzcyński et al. (2001) |
- |
Gaposchkin (1957) |
- |
Kenyon (1986) |
- |
Akras et al. (2019) |
- |
Boyarchuk (1969) |
- |
Vaidis (1988, 1991) |
- |
Position
Right ascension (°) |
162.3661Ref |
Parallax (mas) |
0.373±0.607Ref |
Reddening E(B-V) (mag) |
0.01±0.0Ref, Note |
Declination (°) |
51.0628Ref |
Distance (kpc) |
1.64Ref, Note, 1.57Ref, Note |
|
|
Galactic longitude (°) |
158.5391Ref |
Proper motion in α (mas/yr) |
0.03±0.45Ref |
|
|
Galactic latitude (°) |
56.7877Ref |
Proper motion in δ (mas/yr) |
-1.04±0.66Ref |
|
|
Observations
X-Ray |
YesRef |
IR type |
- |
Radio |
- |
X-Ray type |
βRef |
J (mag) |
- |
Flickering |
- |
GALEX FUV (mag) |
- |
H (mag) |
- |
Outbursts |
- |
GALEX NUV (mag) |
- |
K (mag) |
- |
Outburst type |
- |
IUE |
NoRef |
WISE W1 (mag) |
16.92Ref |
Jets |
- |
FUSE |
NoRef |
WISE W2 (mag) |
16.06Ref |
Resolved nebula |
- |
U (mag) |
- |
WISE W3 (mag) |
12.82Ref |
IPmax (eV) |
- |
B (mag) |
- |
WISE W4 (mag) |
8.73Ref |
[O III] lines |
- |
V (mag) |
- |
IRAS 12μm (Jy) |
- |
He II lines |
- |
R (mag) |
19.92Ref |
IRAS 25μm (Jy) |
- |
[Fe VII] lines |
- |
I (mag) |
- |
IRAS 60μm (Jy) |
- |
O VI lines |
- |
BP (mag) |
20.63Ref |
IRAS 100μm (Jy) |
- |
|
|
G (mag) |
20.37Ref |
AKARI S09 (Jy) |
- |
|
|
RP (mag) |
20.07Ref |
AKARI S18 (Jy) |
- |
|
|
Orbit
Orbital period (days) |
- |
γ velocity (km/h) |
-11.70±2.80Ref |
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 |
- |
Luminosity (L⊙) |
- |
Pulsation period (days) |
- |
Metallicity [Fe/H] |
-1.6Ref |
|
|
Pulsation ephemeris |
- |
Hot component
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) |
- |
|
|
|
|
References
- Martin, N. F., Ibata, R. A., Chapman, S. C. et al., 2007, MNRAS, 380, 1, 281, 2007MNRAS.380..281M
- Saeedi, S., Sasaki, M., 2020, MNRAS, 499, 3, 3111, 2020MNRAS.499.3111S
Last updated: November 12, 2020