SUSPECTED NGC 6822
Equatorial coordinates
α = 296.245780 | 19 44 58.990000
δ = -14.786500 | -14 47 11.400000 |
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Constellation |
Sagittarius |
Symbiotic IR Type |
S |
Spectral Type |
C |
Magnitude range (V) |
|
Outbursts |
No |
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Identifiers
[LDB2002] 513 |
GSC – |
TYC – |
WRAY – |
SIMBAD [LDB2002] 513 |
HIP – |
SAO – |
Hen – |
BD – |
IRAS – |
GAIA DR2 – |
ESO – |
HD – |
2MASS – |
WISE – |
AAVSO – |
Position
Right ascension (°) |
296.245780 |
Parallax (mas) |
– |
Reddening E(B-V) (mag) |
0.199 ± 0.009 |
Declination (°) |
-14.786500 |
Distance (kpc) |
500.00 ± 10.00 |
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Galactic longitude (°) |
25.357957 |
Proper motion in α (mas/yr) |
– |
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Galactic latitude (°) |
-18.396893 |
Proper motion in δ (mas/yr) |
– |
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Observations
U (mag) |
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X-Ray |
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Flickering |
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B (mag) |
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X-Ray type |
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Outbursts |
No |
V (mag) |
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IUE |
No |
Type |
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R (mag) |
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IRAS flux at 12 μm (Jy) |
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IPmax (eV) |
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I (mag) |
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IRAS flux at 25 μm (Jy) |
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OVI lines |
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G (mag) |
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IRAS flux at 60 μm (Jy) |
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J (mag) |
17.58 |
IRAS flux at 100 μm (Jy) |
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H (mag) |
16.73 |
WISE W1 (mag) |
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K (mag) |
16.46 |
WISE W2 (mag) |
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L (mag) |
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WISE W3 (mag) |
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WISE W4 (mag) |
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Radio |
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Radio flux (mJy) |
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Orbit
Orbital period (days) |
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γ velocity (km/h) |
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Size of giant’s orbit (AU) |
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Eccentricity |
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RV of giant (km/h) |
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Separation (AU) |
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Inclination (°) |
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Inferior conj. of giant (JD) |
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Mass function |
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Ephemeris type |
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Mass ratio |
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Ephemeris T0 (JD) |
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Cool component
Spectral type |
C |
Mass (M⊙) |
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Pulsation |
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Eff. temperature (K) |
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Radius (R⊙) |
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Type |
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IR type |
S |
Luminosity (L⊙) |
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Pulsation period (days) |
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Metallicity [Fe/H] |
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Ephemeris type |
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Ephemeris T0 (JD) |
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Hot component
Type/Spectra |
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Mass (M⊙) |
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Spin period (min) |
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Eff. temperature (K) |
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Radius (R⊙) |
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Accretion disk |
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Lower limit (K) |
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Luminosity (L⊙) |
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Upper limit (K) |
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Links
SIMBAD CDS Portal
Notes
It was suspected to be a symbiotic star based on its spectra by Sibbons et al. (2015).
References
- Sibbons, L. F., Ryan, S. G., Napiwotzki, R., et al., 2015, A&A, 574, A102, 2015A&A…574A.102S
Last updated: May 13, 2019 @ 11:18 am