CONFIRMED SMC
Equatorial coordinates
α = 16.163797 ± 0.022927 | 01 04 39.306394
δ = -75.806885 ± 0.019812 | -75 48 24.765843 |
|
Constellation |
Hydrus |
Symbiotic IR Type |
S |
Spectral Type |
K7 |
Magnitude range (V) |
|
Outbursts |
No |
|
|
Identifiers
Position
Right ascension (°) |
16.163797 ± 0.022927 |
Parallax (mas) |
– |
Reddening E(B-V) (mag) |
0.044 ± 0.001 |
Declination (°) |
-75.806885 ± 0.019812 |
Distance (kpc) |
62.10 ± 1.90 |
|
|
Galactic longitude (°) |
301.854131 ± 0.019812 |
Proper motion in α (mas/yr) |
1.158752 ± 0.041509 |
|
|
Galactic latitude (°) |
-41.293699 ± 0.022927 |
Proper motion in δ (mas/yr) |
-1.352465 ± 0.037801 |
|
|
Observations
U (mag) |
|
X-Ray |
No |
Flickering |
|
B (mag) |
17.30 |
X-Ray type |
|
Outbursts |
No |
V (mag) |
15.60 |
IUE |
Yes |
Type |
|
R (mag) |
15.52 |
IRAS flux at 12 μm (Jy) |
|
IPmax (eV) |
114.0 |
I (mag) |
13.88 |
IRAS flux at 25 μm (Jy) |
|
OVI lines |
Yes |
G (mag) |
15.02 |
IRAS flux at 60 μm (Jy) |
|
|
|
J (mag) |
15.55 |
IRAS flux at 100 μm (Jy) |
|
|
|
H (mag) |
11.71 |
WISE W1 (mag) |
11.37 |
|
|
K (mag) |
11.49 |
WISE W2 (mag) |
11.46 |
|
|
L (mag) |
|
WISE W3 (mag) |
11.27 |
|
|
|
|
WISE W4 (mag) |
9.03 |
|
|
|
|
Radio |
|
|
|
|
|
Radio flux (mJy) |
|
|
|
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 |
|
Ephemeris type |
|
|
|
Mass ratio |
|
Ephemeris T0 (JD) |
|
|
|
|
|
Cool component
Spectral type |
K7 |
Mass (M⊙) |
|
Pulsation |
|
Eff. temperature (K) |
3850 |
Radius (R⊙) |
150 |
Type |
|
IR type |
S |
Luminosity (L⊙) |
4500 |
Pulsation period (days) |
|
Metallicity [Fe/H] |
|
|
|
Ephemeris type |
|
|
|
|
|
Ephemeris T0 (JD) |
|
Hot component
Type/Spectra |
|
Mass (M⊙) |
|
Spin period (min) |
|
Eff. temperature (K) |
130000 ± 10000 |
Radius (R⊙) |
0.10 |
Accretion disk |
|
Lower limit (K) |
|
Luminosity (L⊙) |
3000 ± 1000 |
|
|
Upper limit (K) |
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Links
SIMBAD CDS Portal VSX
Notes
Proposed to be a symbiotic star based on a 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
- Muerset, U., Schild, H., Vogel, M., 1996, A&A, 307, 516, 1996A&A…307..516M
- Walker, A. R., 1983, MNRAS, 203, 25, 1983MNRAS.203…25W
Last updated: May 2, 2019 @ 11:27 am