SMC N73
CONFIRMED
SMC
Constellation
Hydrus |
Equatorial coordinates
α = 01 04 39.311
δ = -75 48 24.787 |
Galactic coordinates
l = 301.8541°
b = -41.2937° |
Suspected |
1983Ref |
Confirmed |
1983Ref |
Symbiotic IR type |
SRef |
Hot component type |
shell-burningRef |
Outbursts |
- |
|
|
Symbiotic Catalogs
Bidelman (1954) |
- |
Allen (1984) |
SMC N73 (Conf.) |
Belzcyński et al. (2001) |
SMC N73 (Conf.) |
Gaposchkin (1957) |
- |
Kenyon (1986) |
SMC N73 (Conf.) |
Akras et al. (2019) |
SMC N73 (Conf.) |
Boyarchuk (1969) |
- |
Vaidis (1988, 1991) |
Lin 445a (Conf.) |
Position
Right ascension (°) |
16.1638Ref |
Parallax (mas) |
-0.023±0.019Ref |
Reddening E(B-V) (mag) |
0.04±0.0Ref, Note |
Declination (°) |
-75.8069Ref |
Distance (kpc) |
62.1±1.9Ref 22.52Ref, Note, 20.91Ref, Note |
|
|
Galactic longitude (°) |
301.8541Ref |
Proper motion in α (mas/yr) |
1.18±0.02Ref |
|
|
Galactic latitude (°) |
-41.2937Ref |
Proper motion in δ (mas/yr) |
-1.41±0.02Ref |
|
|
Observations
X-Ray |
NoRef |
IR type |
SRef |
Radio |
- |
X-Ray type |
- |
J (mag) |
12.55Ref |
Flickering |
- |
GALEX FUV (mag) |
19.91Ref |
H (mag) |
11.71Ref |
Outbursts |
- |
GALEX NUV (mag) |
20.53Ref |
K (mag) |
11.49Ref |
Outburst type |
- |
IUE |
NoRef |
WISE W1 (mag) |
11.37Ref |
Jets |
- |
FUSE |
YesRef |
WISE W2 (mag) |
11.46Ref |
Resolved nebula |
- |
U (mag) |
- |
WISE W3 (mag) |
11.27Ref |
IPmax (eV) |
114Ref |
B (mag) |
17.30Ref |
WISE W4 (mag) |
9.03Ref |
[O III] lines |
NoRef |
V (mag) |
15.60Ref |
IRAS 12μm (Jy) |
- |
He II lines |
YesRef |
R (mag) |
15.52Ref |
IRAS 25μm (Jy) |
- |
[Fe VII] lines |
NoRef |
I (mag) |
13.88Ref |
IRAS 60μm (Jy) |
- |
O VI lines |
YesRef |
BP (mag) |
16.02Ref |
IRAS 100μm (Jy) |
- |
|
|
G (mag) |
15.00Ref |
AKARI S09 (Jy) |
- |
|
|
RP (mag) |
14.00Ref |
AKARI S18 (Jy) |
- |
|
|
Orbit
Orbital period (days) |
- |
γ velocity (km/h) |
163.38±3.07Ref |
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 |
11.7?Ref |
Orbital ephemeris |
- |
|
|
|
|
Cool component
Spectral type |
K7Ref |
Mass (M⊙) |
2±0.55Ref |
Pulsation |
- |
Eff. temperature (K) |
3850Ref, 3590±50Ref |
Radius (R⊙) |
150Ref, 208±16Ref |
Type |
- |
IR type |
SRef |
Luminosity (L⊙) |
4500Ref |
Pulsation period (days) |
- |
Metallicity [Fe/H] |
-0.75±0.12Ref |
|
|
Pulsation ephemeris |
- |
Hot component
Type/Spectral type |
WDRef |
Mass (M⊙) |
>0.17Ref |
Spin period (min) |
- |
Shell-burning/Accreting-only |
shell-burningRef |
Radius (R⊙) |
0.1Ref |
Accretion disk |
- |
Eff. temperature (K) |
130000±10000Ref, 200000Ref |
Luminosity (L⊙) |
3000±1000Ref, 14000Ref |
|
|
Lower limit (K) |
- |
|
|
|
|
Upper limit (K) |
- |
|
|
|
|
Notes
The star was proposed to be a symbiotic star based on the visibility of a strong UV continuum with TiO and a strong He II λ4686 emission line.
References
- Morgan, D. H., 1992, MNRAS, 258, 639, 1992MNRAS.258..639M
- Mürset, U., Schild, H., Vogel, M., 1996, A&A, 307, 516, 1996A&A...307..516M
- Walker, A. R., 1983, MNRAS, 203, 25, 1983MNRAS.203...25W
- Washington, J. E., Lewis, H. M., Anguiano, B. et al., 2021, ApJ, 918, 1, 19, 2021ApJ...918...19W
Last updated: August 21, 2021