47 Tuc Src-No. 568
SUSPECTED
MILKY WAY
Constellation
Tucana |
Equatorial coordinates
α = 00 25 57.538
δ = -72 07 52.813 |
Galactic coordinates
l = 305.6846°
b = -44.8605° |
Suspected |
2021Ref |
Confirmed |
- |
Symbiotic IR type |
S?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) |
- |
Boyarchuk (1969) |
- |
Vaidis (1988, 1991) |
- |
Position
Right ascension (°) |
6.4897Ref |
Parallax (mas) |
0.226±0.011Ref |
Reddening E(B-V) (mag) |
0.03±0.0Ref, Note |
Declination (°) |
-72.1313Ref |
Distance (kpc) |
4.40Ref, Note, 4.52Ref, Note |
|
|
Galactic longitude (°) |
305.6846Ref |
Proper motion in α (mas/yr) |
5.66±0.01Ref |
|
|
Galactic latitude (°) |
-44.8605Ref |
Proper motion in δ (mas/yr) |
-2.56±0.01Ref |
|
|
Observations
X-Ray |
YesRef |
IR type |
S?Ref |
Radio |
- |
X-Ray type |
βRef |
J (mag) |
10.42Ref |
Flickering |
- |
GALEX FUV (mag) |
- |
H (mag) |
9.71Ref |
Outbursts |
- |
GALEX NUV (mag) |
- |
K (mag) |
9.58Ref |
Outburst type |
- |
IUE |
NoRef |
WISE W1 (mag) |
9.47Ref |
Jets |
- |
FUSE |
NoRef |
WISE W2 (mag) |
9.61Ref |
Resolved nebula |
- |
U (mag) |
- |
WISE W3 (mag) |
9.47Ref |
IPmax (eV) |
- |
B (mag) |
13.97Ref |
WISE W4 (mag) |
8.53Ref |
[O III] lines |
- |
V (mag) |
12.75Ref |
IRAS 12μm (Jy) |
- |
He II lines |
- |
R (mag) |
12.53Ref |
IRAS 25μm (Jy) |
- |
[Fe VII] lines |
- |
I (mag) |
11.41Ref |
IRAS 60μm (Jy) |
- |
O VI lines |
- |
BP (mag) |
13.05Ref |
IRAS 100μm (Jy) |
- |
|
|
G (mag) |
12.35Ref |
AKARI S09 (Jy) |
- |
|
|
RP (mag) |
11.54Ref |
AKARI S18 (Jy) |
- |
|
|
Orbit
Orbital period (days) |
- |
γ velocity (km/h) |
-17.21±0.51Ref |
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 |
S?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
Suspected in the first version of the paper by Saeedi et al. (2021), based on X-ray detection by eROSITA and a possible RGB counterpart. However, it is not mentioned in the second version.
Last updated: March 25, 2022