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