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 | 
- | 
 
 
   | 
    
      
      
      
     | 
  
     
    
    
      
      
  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) | 
- | 
  | 
  | 
  | 
  | 
 
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
- Allen, D. A., 1980, MNRAS, 192, 521, 1980MNRAS.192..521A
 
- Allen, D. A., 1984, PASA, 5, 3, 369, 1984PASA....5..369A
 
- Gałan, C., Mikołajewska, J., Hinkle, K. H. et al., 2017, MNRAS, 466, 2, 2194, 2017MNRAS.466.2194G
 
- Gromadzki, M., Mikołajewska, J., Soszyński, I., 2013, AcA, 63, 4, 405, 2013AcA....63..405G
 
- Herbig, G. H., 1969, PNAS, 63, 4, 1045, 1969PNAS...63.1045H
 
- Medina Tanco, G. A., Steiner, J. E., 1995, AJ, 109, 1770, 1995AJ....109.1770M
 
- Mikołajewska, J., Acker, A., Stenholm, B., 1997, A&A, 327, 191, 1997A&A...327..191M
 
- Sanduleak, N., Stephenson, C. B., 1973, ApJ, 185, 899, 1973ApJ...185..899S
 
- Stenholm, B., Acker, A., 1987, A&AS, 68, 51, 1987A&AS...68...51S
 
- Toma, R., Ramsay, G., Macfarlane, S. et al., 2016, MNRAS, 463, 1, 1099, 2016MNRAS.463.1099T
 
 
Last updated: April 18, 2022