Hen 3-160
CONFIRMED
MILKY WAY
Constellation
Vela |
Equatorial coordinates
α = 08 24 53.137
δ = -51 28 32.933 |
Galactic coordinates
l = 267.6767°
b = -7.8700° |
Suspected |
1973Ref |
Confirmed |
1978Ref |
Symbiotic IR type |
SRef |
Hot component type |
shell-burningRef |
Outbursts |
- |
|
|
Symbiotic Catalogs
Bidelman (1954) |
- |
Allen (1984) |
Hen 160 (Conf.) |
Belzcyński et al. (2001) |
Hen 3-160 (Conf.) |
Gaposchkin (1957) |
- |
Kenyon (1986) |
Hen 160 (Conf.) |
Akras et al. (2019) |
Hen 3-160 (Conf.) |
Boyarchuk (1969) |
- |
Vaidis (1988, 1991) |
VDS 18 (Conf.) |
Position
Right ascension (°) |
126.2214Ref |
Parallax (mas) |
-0.005±0.038Ref |
Reddening E(B-V) (mag) |
0.54±0.02Ref, Note |
Declination (°) |
-51.4758Ref |
Distance (kpc) |
9.4Ref 10.27Ref, Note, 8.60Ref, Note |
|
|
Galactic longitude (°) |
267.6767Ref |
Proper motion in α (mas/yr) |
-1.24±0.05Ref |
|
|
Galactic latitude (°) |
-7.8700Ref |
Proper motion in δ (mas/yr) |
2.85±0.04Ref |
|
|
Observations
X-Ray |
NoRef |
IR type |
SRef |
Radio |
NoRef |
X-Ray type |
- |
J (mag) |
9.30Ref |
Flickering |
NoRef |
GALEX FUV (mag) |
- |
H (mag) |
8.33Ref |
Outbursts |
- |
GALEX NUV (mag) |
- |
K (mag) |
7.80Ref |
Outburst type |
- |
IUE |
NoRef |
WISE W1 (mag) |
7.55Ref |
Jets |
- |
FUSE |
NoRef |
WISE W2 (mag) |
7.27Ref |
Resolved nebula |
- |
U (mag) |
- |
WISE W3 (mag) |
6.55Ref |
IPmax (eV) |
114Ref |
B (mag) |
16.14Ref |
WISE W4 (mag) |
6.02Ref |
[O III] lines |
YesRef |
V (mag) |
15.64Ref |
IRAS 12μm (Jy) |
- |
He II lines |
YesRef |
R (mag) |
- |
IRAS 25μm (Jy) |
- |
[Fe VII] lines |
YesRef |
I (mag) |
- |
IRAS 60μm (Jy) |
- |
O VI lines |
YesRef |
BP (mag) |
14.58Ref |
IRAS 100μm (Jy) |
- |
|
|
G (mag) |
13.54Ref |
AKARI S09 (Jy) |
0.13Ref |
|
|
RP (mag) |
11.97Ref |
AKARI S18 (Jy) |
- |
|
|
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 |
M7 IIIRef, M3.5(max)Ref, M8(min)Ref |
Mass (M⊙) |
- |
Pulsation |
YesRef |
Eff. temperature (K) |
3000-3500Ref, 2770Ref |
Radius (R⊙) |
- |
Type |
MiraRef |
IR type |
SRef |
Luminosity (L⊙) |
3960Ref |
Pulsation period (days) |
242.53±0.14Ref |
Metallicity [Fe/H] |
- |
|
|
Pulsation ephemeris |
- |
Hot component
Type/Spectral type |
- |
Mass (M⊙) |
- |
Spin period (min) |
- |
Shell-burning/Accreting-only |
shell-burningRef |
Radius (R⊙) |
- |
Accretion disk |
- |
Eff. temperature (K) |
- |
Luminosity (L⊙) |
1020Ref |
|
|
Lower limit (K) |
114000Ref |
|
|
|
|
Upper limit (K) |
200000Ref |
|
|
|
|
Notes
This star is the first symbiotic binary with Mira variable S star (Gałan et al., 2019).
References
- Gałan, C., Mikołajewska, J., Monard, B. et al., 2019, AcA, 69, 1, 25, 2019AcA....69...25G
- Merc, J., Beck, P. G., Mathur, S. et al., 2023, arXiv, arXiv:2312.16126, 2023arXiv231216126M
Last updated: January 13, 2024