AS 288

LIKELY MILKY WAY
 
Constellation
Sagittarius
Equatorial coordinates
α = 18 12 47.981
δ = -28 19 59.807
Galactic coordinates
l = 3.4920°
b = -4.8740°

Suspected 1978Ref
Confirmed -
Symbiotic IR type D?Ref
Hot component type shell-burning?Ref
Outbursts -

Identifiers

AS 288 IRAS 18095-2820 GSC2.4.2 S9TL016082 AAVSO 000-BJT-866
SIMBAD PN H 2-43 Pan-STARRS 74002731999410398 SAO - VSX 241105
GAIA DR3 4050670827750135040 SkyMapper - WRAY 16-388 GCVS -
2MASS J18124799-2819596 HIP - Hen 2-366 BD -
WISE J181247.98-281959.7 TYC - ESO 456-75 HD -

Symbiotic Catalogs

Bidelman (1954) - Allen (1984) - Belzcyński et al. (2001) AS 288 (Susp.)
Gaposchkin (1957) - Kenyon (1986) - Akras et al. (2019) AS 288 (Susp.)
Boyarchuk (1969) - Vaidis (1988, 1991) -

Position

Right ascension (°) 273.1999Ref Parallax (mas) 0.126±0.028Ref Reddening E(B-V) (mag) 0.42±0.02Ref, Note
Declination (°) -28.3333Ref Distance (kpc) 6.34Ref, Note, 6.29Ref, Note    
Galactic longitude (°) 3.4920Ref Proper motion in α (mas/yr) -4.03±0.03Ref    
Galactic latitude (°) -4.8740Ref Proper motion in δ (mas/yr) -4.07±0.02Ref    

Observations

X-Ray NoRef IR type D?Ref Radio NoRef, YesRef
X-Ray type - J (mag) 11.47Ref Flickering -
GALEX FUV (mag) - H (mag) 9.75Ref Outbursts -
GALEX NUV (mag) - K (mag) 8.31Ref Outburst type -
IUE NoRef WISE W1 (mag) 6.76Ref Jets -
FUSE NoRef WISE W2 (mag) 5.82Ref Resolved nebula -
U (mag) - WISE W3 (mag) 4.06Ref IPmax (eV) 54.4Ref
B (mag) 12.00Ref WISE W4 (mag) 2.73Ref [O III] lines -
V (mag) 14.20Ref IRAS 12μm (Jy) 1.24Ref He II lines YesRef
R (mag) - IRAS 25μm (Jy) 1.10Ref [Fe VII] lines NoRef
I (mag) - IRAS 60μm (Jy) 4.33Ref O VI lines NoRef
BP (mag) 14.03Ref IRAS 100μm (Jy) 49.30Ref
G (mag) 13.62Ref AKARI S09 (Jy) 0.80Ref
RP (mag) 12.85Ref AKARI S18 (Jy) 0.70Ref

Orbit

Orbital period (days) 1250Ref 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 -
Eclipses -     Mass ratio -
Orbital ephemeris -        

Cool component

Spectral type - Mass (M) - Pulsation -
Eff. temperature (K) - Radius (R) - Type -
IR type D?Ref Luminosity (L) - Pulsation period (days) -
Metallicity [Fe/H] -     Pulsation ephemeris -

Hot component

Type/Spectral type - Mass (M) - Spin period (min) -
Shell-burning/Accreting-only shell-burning?Ref Radius (R) - Accretion disk -
Eff. temperature (K) - Luminosity (L) -    
Lower limit (K) -        
Upper limit (K) -        

Links

SIMBAD   CDS Portal


Notes

Mentioned as a symbiotic star in Wright & Allen (1978). List as a suspected symbiotic binary in Belczyński et al. (2000). Its spectrum exhibits emission-lines with ionization potential up to 54.4 eV, but no late-type giant. In the IR diagram, it is situated among D-type symbiotic stars. The symbiotic nature is further supported by the analysis of IR data by Akras et al. (2019).


References


Last updated: August 20, 2021