HK Sco
CONFIRMED
MILKY WAY
Constellation
Scorpius |
Equatorial coordinates
α = 16 54 41.036
δ = -30 23 06.979 |
Galactic coordinates
l = 352.4854°
b = 8.2663° |
Suspected |
1941Ref |
Confirmed |
1941Ref |
Symbiotic IR type |
SRef |
Hot component type |
shell-burningRef |
Outbursts |
YesRef - Z AndRef |
|
|
Symbiotic Catalogs
Bidelman (1954) |
HK Sco (Conf.) |
Allen (1984) |
HK Sco (Conf.) |
Belzcyński et al. (2001) |
HK Sco (Conf.) |
Gaposchkin (1957) |
HK Sco (Conf.) |
Kenyon (1986) |
HK Sco (Conf.) |
Akras et al. (2019) |
HK Sco (Conf.) |
Boyarchuk (1969) |
HK Sco (Susp.) |
Vaidis (1988, 1991) |
HK Sco (Conf.) |
Position
Right ascension (°) |
253.6710Ref |
Parallax (mas) |
0.098±0.022Ref |
Reddening E(B-V) (mag) |
0.31±0.01Ref, Note |
Declination (°) |
-30.3853Ref |
Distance (kpc) |
2.8Ref 8.79Ref, Note, 7.16Ref, Note |
|
|
Galactic longitude (°) |
352.4854Ref |
Proper motion in α (mas/yr) |
-3.09±0.03Ref |
|
|
Galactic latitude (°) |
8.2663Ref |
Proper motion in δ (mas/yr) |
-6.04±0.02Ref |
|
|
Observations
X-Ray |
NoRef |
IR type |
SRef |
Radio |
NoRef |
X-Ray type |
- |
J (mag) |
9.02Ref |
Flickering |
NoRef |
GALEX FUV (mag) |
- |
H (mag) |
8.12Ref |
Outbursts |
YesRef |
GALEX NUV (mag) |
- |
K (mag) |
7.70Ref |
Outburst type |
Z AndRef |
IUE |
NoRef |
WISE W1 (mag) |
7.70Ref |
Jets |
- |
FUSE |
NoRef |
WISE W2 (mag) |
7.69Ref |
Resolved nebula |
- |
U (mag) |
- |
WISE W3 (mag) |
7.37Ref |
IPmax (eV) |
114Ref |
B (mag) |
15.35Ref |
WISE W4 (mag) |
6.83Ref |
[O III] lines |
NoRef |
V (mag) |
13.84Ref |
IRAS 12μm (Jy) |
- |
He II lines |
YesRef |
R (mag) |
- |
IRAS 25μm (Jy) |
- |
[Fe VII] lines |
NoRef |
I (mag) |
- |
IRAS 60μm (Jy) |
- |
O VI lines |
YesRef |
BP (mag) |
13.65Ref |
IRAS 100μm (Jy) |
- |
|
|
G (mag) |
12.27Ref |
AKARI S09 (Jy) |
- |
|
|
RP (mag) |
11.08Ref |
AKARI S18 (Jy) |
- |
|
|
Orbit
Orbital period (days) |
458±21Ref |
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 |
NoRef |
|
|
Mass ratio |
- |
Orbital ephemeris |
Min (V) = 2452023 + 458±21 x ERef |
|
|
|
|
Cool component
Spectral type |
M1 IIIRef, M1 IIIRef, M3.5 IIIRef |
Mass (M⊙) |
- |
Pulsation |
- |
Eff. temperature (K) |
3790Ref |
Radius (R⊙) |
- |
Type |
- |
IR type |
SRef |
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-burningRef |
Radius (R⊙) |
- |
Accretion disk |
- |
Eff. temperature (K) |
65000-100000Ref |
Luminosity (L⊙) |
- |
|
|
Lower limit (K) |
- |
|
|
|
|
Upper limit (K) |
- |
|
|
|
|
Notes
Elvey (1941) reported a faint continuous spectrum with Balmer lines and He II. Additionally, Swope (1941) observed variability in the star, including outbursts.
References
- Allen, D. A., 1978, MNRAS, 184, 601, 1978MNRAS.184..601A
- Allen, D. A., 1980, MNRAS, 192, 521, 1980MNRAS.192..521A
- Elvey, C. T., 1941, ApJ, 94, 140, 1941ApJ....94..140E
- Gromadzki, M., Mikołajewska, J., Soszyński, I., 2013, AcA, 63, 4, 405, 2013AcA....63..405G
- Medina Tanco, G. A., Steiner, J. E., 1995, AJ, 109, 1770, 1995AJ....109.1770M
- Merc, J., Beck, P. G., Mathur, S. et al., 2023, arXiv, arXiv:2312.16126, 2023arXiv231216126M
- Mürset, U., Schmid, H. M., 1999, A&AS, 137, 473, 1999A&AS..137..473M
- Sanduleak, N., Stephenson, C. B., 1973, ApJ, 185, 899, 1973ApJ...185..899S
- Swope, H. H., 1941, ApJ, 94, 140, 1941ApJ....94..140S
Last updated: January 13, 2024