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

Identifiers

Gaia18aen IRAS - GSC2.4.2 S64K095761 AAVSO 000-BMR-246
SIMBAD WRAY 15-136 Pan-STARRS 71621207168887856 SAO - VSX 424655
GAIA DR3 5596273362288326912 SkyMapper 080252.06-301837.2 WRAY 15-136 GCVS -
2MASS J08025205-3018373 HIP - Hen - BD -
WISE J080252.06-301837.1 TYC - ESO - HD -

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        

Links

SIMBAD   CDS Portal


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


Last updated: April 12, 2021