IV Vir
        
      
        
  
    
    
    CONFIRMED
    MILKY WAY  
    
Constellation 
Virgo | 
Equatorial coordinates 
α = 14 16 34.293 
δ =  -21 45 50.315 | 
Galactic coordinates 
l = 327.8816°  
b = 36.9490°  | 
 
  
| Suspected | 
1973Ref | 
 
| Confirmed | 
1984Ref | 
 
| Symbiotic IR type | 
SRef | 
 
| Hot component type | 
shell-burningRef | 
 
| Outbursts | 
- | 
 
 
   | 
    
      
      
      
     | 
  
     
    
    
      
      
  Symbiotic Catalogs
  
| Bidelman (1954) | 
- | 
Allen (1984) | 
BD-21.3873 (Conf.) | 
Belzcyński et al. (2001) | 
BD-21 3873 (Conf.) | 
| Gaposchkin (1957) | 
- | 
Kenyon (1986) | 
BD-21°3873 (Conf.) | 
Akras et al. (2019) | 
BD-21 3873 (Conf.) | 
| Boyarchuk (1969) | 
- | 
Vaidis (1988, 1991) | 
-21°3873 (Conf.) | 
   
  
  
Position
| Right ascension (°) | 
214.1429Ref | 
Parallax (mas) | 
0.251±0.018Ref | 
Reddening E(B-V) (mag) | 
0.11±0.0Ref, Note | 
| Declination (°) | 
-21.7640Ref | 
Distance (kpc) | 
1.3Ref 3.53Ref, Note, 3.28Ref, Note | 
  | 
  | 
| Galactic longitude (°) | 
327.8816Ref | 
Proper motion in α (mas/yr) | 
1.64±0.02Ref | 
  | 
  | 
| Galactic latitude (°) | 
36.9490Ref | 
Proper motion in δ (mas/yr) | 
-17.39±0.02Ref | 
  | 
  | 
 
  
  
Observations
  
     | X-Ray | 
     NoRef | 
     IR type | 
     SRef | 
     Radio | 
     NoRef | 
   
   
     | X-Ray type | 
     - | 
     J (mag) | 
     8.12Ref | 
     Flickering | 
     NoRef | 
   
   
     | GALEX FUV (mag) | 
     13.95Ref | 
     H (mag) | 
     7.32Ref | 
     Outbursts | 
     - | 
   
   
     | GALEX NUV (mag) | 
     14.51Ref | 
     K (mag) | 
     7.13Ref | 
     Outburst type | 
     - | 
   
   
     | IUE | 
     YesRef | 
     WISE W1 (mag) | 
     6.98Ref | 
     Jets | 
     - | 
   
   
     | FUSE | 
     NoRef | 
     WISE W2 (mag) | 
     6.97Ref | 
     Resolved nebula | 
     NoRef | 
   
   
     | U (mag) | 
     - | 
     WISE W3 (mag) | 
     6.73Ref | 
     IPmax (eV) | 
     77.5Ref | 
   
   
     | B (mag) | 
     12.06Ref | 
     WISE W4 (mag) | 
     6.15Ref | 
     [O III] lines | 
     NoRef | 
   
   
     | V (mag) | 
     10.68Ref | 
     IRAS 12μm (Jy) | 
     - | 
     He II lines | 
     YesRef | 
   
   
     | R (mag) | 
     - | 
     IRAS 25μm (Jy) | 
     - | 
     [Fe VII] lines | 
     NoRef | 
   
   
     | I (mag) | 
     - | 
     IRAS 60μm (Jy) | 
     - | 
     O VI lines | 
     NoRef | 
   
   
     | BP (mag) | 
     11.00Ref | 
     IRAS 100μm (Jy) | 
     - | 
      | 
      | 
   
   
     | G (mag) | 
     10.18Ref | 
     AKARI S09 (Jy) | 
     - | 
      | 
      | 
   
   
     | RP (mag) | 
     9.30Ref | 
     AKARI S18 (Jy) | 
     - | 
      | 
      | 
   
 
Orbit
| Orbital period (days) | 
281.6±1.2Ref | 
γ velocity (km/h) | 
203.9±0.2Ref, 23.56±2.86Ref | 
Size of giant’s orbit (AU) | 
0.276Ref | 
| Eccentricity | 
0Ref | 
RV of giant (km/h) | 
10.6±0.3Ref | 
Separation (AU) | 
- | 
| Inclination (°) | 
68Ref | 
Inferior conj. of giant (JD) | 
2449087.3 | 
Mass function | 
0.035Ref | 
| Eclipses | 
- | 
  | 
  | 
Mass ratio | 
2Ref | 
| Orbital ephemeris | 
- | 
  | 
  | 
  | 
  | 
 
Cool component
| Spectral type | 
G8 IIIRef, K2 IIIRef | 
Mass (M⊙) | 
0.9Ref | 
Pulsation | 
- | 
| Eff. temperature (K) | 
4300Ref, 4420±100Ref,  4100Ref | 
Radius (R⊙) | 
37Ref, 20.8Ref | 
Type | 
- | 
| IR type | 
SRef | 
Luminosity (L⊙) | 
780Ref, 190Ref | 
Pulsation period (days) | 
- | 
| Metallicity [Fe/H] | 
-1.34Ref, -1.06±0.17Ref | 
  | 
  | 
Pulsation ephemeris | 
- | 
 
Hot component
| Type/Spectral type | 
- | 
Mass (M⊙) | 
0.45Ref | 
Spin period (min) | 
- | 
  | Shell-burning/Accreting-only | 
  shell-burningRef | 
Radius (R⊙) | 
- | 
Accretion disk | 
- | 
  | Eff. temperature (K) | 
  75000Ref | 
Luminosity (L⊙) | 
- | 
  | 
  | 
  | Lower limit (K) | 
  - | 
  | 
  | 
  | 
  | 
| Upper limit (K) | 
- | 
  | 
  | 
  | 
  | 
 
Notes
Bidelman & Macconnell (1973) reported the presence of Balmer and He II lines. The cool component was subsequently classified as a G-type by Allen (1980). Smith et al. (1997) suggested that this star is a twin of AG Dra in terms of metallicities, carbon overabundances, and s-process abundance distributions.
 
References
- Allen, D. A., 1980, MNRAS, 192, 521, 1980MNRAS.192..521A
 
- Allen, D. A., 1984, PASA, 5, 3, 369, 1984PASA....5..369A
 
- Bidelman, W. P., Macconnell, D. J., 1973, AJ, 78, 687, 1973AJ.....78..687B
 
- Merc, J., Beck, P. G., Mathur, S. et al., 2023, arXiv, arXiv:2312.16126, 2023arXiv231216126M
 
- Munari, U., Henden, A., Frigo, A. et al., 2014, AJ, 148, 5, 81, 2014AJ....148...81M
 
- Mürset, U., Schmid, H. M., 1999, A&AS, 137, 473, 1999A&AS..137..473M
 
- Niehues, M., Bruch, A., Duerbeck, H. W., 1992, The Messenger, 67, 38, 1992Msngr..67...38N
 
- Pereira, C. B., Porto de Mello, G. F., 1997, AJ, 114, 2128, 1997AJ....114.2128P
 
- Schmid, H. M., Nussbaumer, H., 1993, A&A, 268, 159, 1993A&A...268..159S
 
- Schulte-Ladbeck, R. E., 1988, A&A, 189, 97, 1988A&A...189...97S
 
- Skopal, A., 2005, A&A, 440, 3, 995, 2005A&A...440..995S
 
- Smith, V. V., Cunha, K., Jorissen, A. et al., 1997, A&A, 324, 97, 1997A&A...324...97S
 
 
Last updated: January 13, 2024