AS 327

CONFIRMED MILKY WAY
 
Constellation
Sagittarius
Equatorial coordinates
α = 18 53 16.658
δ = -24 22 58.845
Galactic coordinates
l = 11.1428°
b = -11.2303°

Suspected 1967Ref
Confirmed 1969Ref
Symbiotic IR type SRef
Hot component type shell-burningRef
Outbursts -

Identifiers

AS 327 IRAS - GSC2.4.2 S9QO000384 AAVSO 000-BDB-940
SIMBAD EM* AS 327 Pan-STARRS 78742833193640683 SAO - VSX 239259
GAIA DR3 4074885853134071936 SkyMapper 185316.65-242258.7 WRAY 16-421 GCVS -
2MASS J18531666-2422588 HIP - Hen 3-1730 BD -
WISE J185316.65-242258.7 TYC - ESO - HD -

Symbiotic Catalogs

Bidelman (1954) - Allen (1984) AS 327 (Conf.) Belzcyński et al. (2001) AS 327 (Conf.)
Gaposchkin (1957) - Kenyon (1986) AS 327 (Conf.) Akras et al. (2019) AS 327 (Conf.)
Boyarchuk (1969) - Vaidis (1988, 1991) MHA 208-67 (Conf.)

Position

Right ascension (°) 283.3194Ref Parallax (mas) 0.149±0.023Ref Reddening E(B-V) (mag) 0.41±0.01Ref, Note
Declination (°) -24.3830Ref Distance (kpc) 3Ref
5.88Ref, Note, 5.47Ref, Note
   
Galactic longitude (°) 11.1428Ref Proper motion in α (mas/yr) -4.21±0.03Ref    
Galactic latitude (°) -11.2303Ref Proper motion in δ (mas/yr) -2.73±0.02Ref    

Observations

X-Ray NoRef IR type SRef Radio YesRef
X-Ray type - J (mag) 8.83Ref Flickering -
GALEX FUV (mag) 17.19Ref H (mag) 7.87Ref Outbursts -
GALEX NUV (mag) 16.70Ref K (mag) 7.55Ref Outburst type -
IUE NoRef WISE W1 (mag) 7.45Ref Jets -
FUSE NoRef WISE W2 (mag) 7.43Ref Resolved nebula -
U (mag) - WISE W3 (mag) 7.02Ref IPmax (eV) 114Ref
B (mag) 14.74Ref WISE W4 (mag) 6.24Ref [O III] lines NoRef
V (mag) 13.09Ref IRAS 12μm (Jy) - He II lines YesRef
R (mag) - IRAS 25μm (Jy) - [Fe VII] lines NoRef
I (mag) - IRAS 60μm (Jy) - O VI lines YesRef
BP (mag) 13.07Ref IRAS 100μm (Jy) -
G (mag) 11.81Ref AKARI S09 (Jy) -
RP (mag) 10.65Ref AKARI S18 (Jy) -

Orbit

Orbital period (days) 823±55Ref γ velocity (km/h) 8.81±2.70Ref 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 Min (V) = 2451954 + 823±55 x ERef        

Cool component

Spectral type M4 IIIRef, M0 IIIRef,
M2 IIIRef
Mass (M) - Pulsation YesRef
Eff. temperature (K) 3560Ref Radius (R) - Type SRRef
IR type SRef Luminosity (L) - Pulsation period (days) 83±1Ref
Metallicity [Fe/H] -     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) 2700Ref    
Lower limit (K) 114000Ref        
Upper limit (K) -        

Links

SIMBAD   CDS Portal   ARAS Database


Notes

Herbig (1969) reported that the object has an early M-type spectrum with bright H and He II lines.


References


Last updated: April 18, 2022