CONFIRMED NGC 6822
Equatorial coordinates
α = 296.224498 ± 0.958948 | 19 44 53.880000
δ = -14.863099 ± 0.987261 | -14 51 46.600000 |
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Constellation |
Sagittarius |
Symbiotic IR Type |
S |
Spectral Type |
Carbon star |
Magnitude range (V) |
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Outbursts |
No |
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Identifiers
Position
Right ascension (°) |
296.224498 ± 0.958948 |
Parallax (mas) |
– |
Reddening E(B-V) (mag) |
0.215 ± 0.009 |
Declination (°) |
-14.863099 ± 0.987261 |
Distance (kpc) |
500.00 ± 10.00 |
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Galactic longitude (°) |
25.275570 ± 0.987261 |
Proper motion in α (mas/yr) |
– |
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Galactic latitude (°) |
-18.409390 ± 0.958948 |
Proper motion in δ (mas/yr) |
– |
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Observations
U (mag) |
22.64 |
X-Ray |
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Flickering |
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B (mag) |
22.82 |
X-Ray type |
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Outbursts |
No |
V (mag) |
21.62 |
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) |
114.0 |
I (mag) |
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IRAS flux at 25 μm (Jy) |
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OVI lines |
Yes |
G (mag) |
20.39 |
IRAS flux at 60 μm (Jy) |
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J (mag) |
17.34 |
IRAS flux at 100 μm (Jy) |
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H (mag) |
16.37 |
WISE W1 (mag) |
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K (mag) |
15.82 |
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 |
Yes |
Eff. temperature (K) |
3318 |
Radius (R⊙) |
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Type |
SR pulsations |
IR type |
S |
Luminosity (L⊙) |
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Pulsation period (days) |
142 ± 3 |
Metallicity [Fe/H] |
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Ephemeris type |
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Ephemeris T0 (JD) |
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Hot component
Type/Spectra |
WD? |
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) |
130000 |
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Links
SIMBAD CDS Portal
Notes
It is an S-type symbiotic star, comprising a red giant losing mass to a compact companion, which is most probably a white dwarf. The red giant is an asymptotic giant branch (AGB) carbon star, and a semiregular variable, pulsating in the first overtone with a period of 142 d (Kniazev et al., 2009).
References
- Akras, S., Guzman-Ramirez, L., Leal-Ferreira, M. L., et al., 2019, ApJS, 240, 21, 2019ApJS..240…21A
- Massey, P., McNeill, R. T., Olsen, K. A. G., et al., 2007, AJ, 134, 2474, 2007AJ….134.2474M
- Kniazev, A. Y., Väisänen, P., Whitelock, P. A., et al., 2009, MNRAS, 395, 1121, 2009MNRAS.395.1121K
Last updated: May 2, 2019 @ 11:15 am