AS 281

CONFIRMED MILKY WAY
 
Constellation
Sagittarius
Equatorial coordinates
α = 18 10 43.858
δ = -27 57 50.145
Galactic coordinates
l = 3.6002°
b = -4.2972°

Suspected 1969Ref
Confirmed 1984Ref
Symbiotic IR type SRef
Hot component type shell-burningRef
Outbursts -

Identifiers

AS 281 IRAS - GSC2.4.2 S9TL001042 AAVSO 000-BJT-854
SIMBAD EM* AS 281 Pan-STARRS 74442726827453643 SAO - VSX 241081
GAIA DR3 4050929693788352384 SkyMapper 181043.88-275749.8 WRAY 16-378 GCVS -
2MASS J18104386-2757501 HIP - Hen 2-357 BD -
WISE J181043.85-275750.0 TYC - ESO 456-65 HD -

Symbiotic Catalogs

Bidelman (1954) - Allen (1984) AS 281 (Conf.) Belzcyński et al. (2001) AS 281 (Conf.)
Gaposchkin (1957) - Kenyon (1986) AS 281 (Conf.) Akras et al. (2019) AS 281 (Conf.)
Boyarchuk (1969) - Vaidis (1988, 1991) Ap1-10 (Conf.)

Position

Right ascension (°) 272.6827Ref Parallax (mas) 0.209±0.041Ref Reddening E(B-V) (mag) 0.48±0.03Ref, Note
Declination (°) -27.9639Ref Distance (kpc) 7Ref, 4.5Ref
5.02Ref, Note, 4.38Ref, Note
   
Galactic longitude (°) 3.6002Ref Proper motion in α (mas/yr) -3.47±0.04Ref    
Galactic latitude (°) -4.2972Ref Proper motion in δ (mas/yr) -2.53±0.03Ref    

Observations

X-Ray NoRef IR type SRef Radio YesRef
X-Ray type - J (mag) 8.30Ref Flickering -
GALEX FUV (mag) - H (mag) 7.28Ref Outbursts -
GALEX NUV (mag) - K (mag) 6.92Ref Outburst type -
IUE NoRef WISE W1 (mag) 6.69Ref Jets -
FUSE NoRef WISE W2 (mag) 6.80Ref Resolved nebula -
U (mag) - WISE W3 (mag) 6.50Ref IPmax (eV) 114Ref
B (mag) 12.00Ref WISE W4 (mag) 6.09Ref [O III] lines NoRef
V (mag) 13.60Ref IRAS 12μm (Jy) - He II lines YesRef
R (mag) - IRAS 25μm (Jy) - [Fe VII] lines YesRef
I (mag) - IRAS 60μm (Jy) - O VI lines YesRef
BP (mag) 14.00Ref IRAS 100μm (Jy) -
G (mag) 12.13Ref AKARI S09 (Jy) -
RP (mag) 10.76Ref AKARI S18 (Jy) -

Orbit

Orbital period (days) 533±30Ref γ velocity (km/h) -137.23±1.01Ref 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 (B) = 2449021 + 533±30 x ERef        

Cool component

Spectral type M5.5 IIIRef, M5 IIIRef,
M3 IIIRef, M6 IIIRef
Mass (M) - Pulsation YesRef
Eff. temperature (K) 3430Ref, 3300Ref Radius (R) - Type SRRef
IR type SRef Luminosity (L) - Pulsation period (days) 65±1Ref
Metallicity [Fe/H] -0.36±0.08Ref     Pulsation ephemeris -

Hot component

Type/Spectral type WDRef Mass (M) - Spin period (min) 31.4Ref
Shell-burning/Accreting-only shell-burningRef Radius (R) - Accretion disk -
Eff. temperature (K) - Luminosity (L) 2800Ref    
Lower limit (K) 114000Ref        
Upper limit (K) -        

Links

SIMBAD   CDS Portal


Notes

Herbig (1969) reported a strong continuous spectrum with intense Hβ and He II. Stenholm & Acker (1987) detected [Fe VII] and O VI lines. Toma et al. (2016) identified variability with a period of 31.4 minutes and an amplitude of 0.008 mag. It might represent a rotational period of a magnetic white dwarf, similar to Z And.


References


Last updated: April 18, 2022