Gaia18aen
CONFIRMED
MILKY WAY
Constellation
Puppis |
Equatorial coordinates
α = 08 02 52.058
δ = -30 18 37.128 |
Galactic coordinates
l = 247.6741°
b = 0.3140° |
Suspected |
2020Ref |
Confirmed |
2020Ref |
Symbiotic IR type |
SRef |
Hot component type |
shell-burningRef |
Outbursts |
YesRef - Z AndRef |
|
|
Symbiotic Catalogs
Bidelman (1954) |
- |
Allen (1984) |
- |
Belzcyński et al. (2001) |
- |
Gaposchkin (1957) |
- |
Kenyon (1986) |
- |
Akras et al. (2019) |
- |
Boyarchuk (1969) |
- |
Vaidis (1988, 1991) |
- |
Position
Right ascension (°) |
120.7169Ref |
Parallax (mas) |
0.264±0.022Ref |
Reddening E(B-V) (mag) |
0.98±0.03Ref, Note |
Declination (°) |
-30.3103Ref |
Distance (kpc) |
6Ref 3.89Ref, Note, 3.95Ref, Note |
|
|
Galactic longitude (°) |
247.6741Ref |
Proper motion in α (mas/yr) |
-1.77±0.02Ref |
|
|
Galactic latitude (°) |
0.3140Ref |
Proper motion in δ (mas/yr) |
4.25±0.02Ref |
|
|
Observations
X-Ray |
NoRef |
IR type |
SRef |
Radio |
- |
X-Ray type |
- |
J (mag) |
8.52Ref |
Flickering |
- |
GALEX FUV (mag) |
- |
H (mag) |
7.19Ref |
Outbursts |
YesRef |
GALEX NUV (mag) |
- |
K (mag) |
6.68Ref |
Outburst type |
Z AndRef |
IUE |
NoRef |
WISE W1 (mag) |
6.39Ref |
Jets |
- |
FUSE |
NoRef |
WISE W2 (mag) |
6.24Ref |
Resolved nebula |
- |
U (mag) |
- |
WISE W3 (mag) |
6.13Ref |
IPmax (eV) |
114Ref |
B (mag) |
15.91Ref |
WISE W4 (mag) |
5.88Ref |
[O III] lines |
YesRef |
V (mag) |
14.20Ref |
IRAS 12μm (Jy) |
- |
He II lines |
YesRef |
R (mag) |
14.10Ref |
IRAS 25μm (Jy) |
- |
[Fe VII] lines |
YesRef |
I (mag) |
14.10Ref |
IRAS 60μm (Jy) |
- |
O VI lines |
YesRef |
BP (mag) |
14.47Ref |
IRAS 100μm (Jy) |
- |
|
|
G (mag) |
12.42Ref |
AKARI S09 (Jy) |
0.22Ref |
|
|
RP (mag) |
11.09Ref |
AKARI S18 (Jy) |
- |
|
|
Orbit
Orbital period (days) |
486.9±3.9Ref |
γ velocity (km/h) |
98.60±0.39Ref |
Size of giant’s orbit (AU) |
- |
Eccentricity |
- |
RV of giant (km/h) |
- |
Separation (AU) |
1.5 - 1.7Ref |
Inclination (°) |
- |
Inferior conj. of giant (JD) |
- |
Mass function |
- |
Eclipses |
NoRef |
|
|
Mass ratio |
- |
Orbital ephemeris |
Min (I) = 2457349.4±8.3 + 486.9±3.9 x ERef |
|
|
|
|
Cool component
Spectral type |
MRef |
Mass (M⊙) |
- |
Pulsation |
Yes?Ref |
Eff. temperature (K) |
3500Ref |
Radius (R⊙) |
230Ref |
Type |
SR or OGLE Small Amplitude Red Giant?Ref |
IR type |
SRef |
Luminosity (L⊙) |
7400Ref |
Pulsation period (days) |
- |
Metallicity [Fe/H] |
0.25Ref |
|
|
Pulsation ephemeris |
- |
Hot component
Type/Spectral type |
WDRef |
Mass (M⊙) |
- |
Spin period (min) |
- |
Shell-burning/Accreting-only |
shell-burningRef |
Radius (R⊙) |
- |
Accretion disk |
- |
Eff. temperature (K) |
- |
Luminosity (L⊙) |
5200-29600Ref |
|
|
Lower limit (K) |
114000Ref |
|
|
|
|
Upper limit (K) |
155000Ref |
|
|
|
|
Notes
Detected in the outburst in 2018. Subsequent spectroscopic and photometric observations presented by Merc et al. (2020) confirmed the object to be the first-ever symbiotic star discovered by the Gaia satellite.
References
- Merc, J., Mikołajewska, J., Gromadzki, M. et al., 2020, A&A, 644, A49, 2020A&A...644A..49M
Last updated: April 12, 2021