V5759 Sgr
CONFIRMED
MILKY WAY
Constellation
Sagittarius |
Equatorial coordinates
α = 18 05 33.728
δ = -20 20 38.225 |
Galactic coordinates
l = 9.7015°
b = 0.4239° |
Suspected |
1950Ref |
Confirmed |
1978Ref |
Symbiotic IR type |
SRef |
Hot component type |
shell-burningRef |
Outbursts |
YesRef - Z AndRef |
|
|
Symbiotic Catalogs
Bidelman (1954) |
F 6-7 (Conf.) |
Allen (1984) |
AS 270 (Conf.) |
Belzcyński et al. (2001) |
AS 270 (Conf.) |
Gaposchkin (1957) |
F 6-7 (Conf.) |
Kenyon (1986) |
AS 270 (Conf.) |
Akras et al. (2019) |
AS 270 (Conf.) |
Boyarchuk (1969) |
F 6-7 (Susp.) |
Vaidis (1988, 1991) |
VDS 116 (Conf.) |
Position
Right ascension (°) |
271.3905Ref |
Parallax (mas) |
0.393±0.041Ref |
Reddening E(B-V) (mag) |
7.28±0.62Ref, Note |
Declination (°) |
-20.3440Ref |
Distance (kpc) |
0.7Ref, 1.1Ref 2.46Ref, Note, 2.47Ref, Note |
|
|
Galactic longitude (°) |
9.7015Ref |
Proper motion in α (mas/yr) |
-1.26±0.05Ref |
|
|
Galactic latitude (°) |
0.4239Ref |
Proper motion in δ (mas/yr) |
-9.63±0.04Ref |
|
|
Observations
X-Ray |
NoRef |
IR type |
SRef |
Radio |
YesRef |
X-Ray type |
- |
J (mag) |
7.21Ref |
Flickering |
- |
GALEX FUV (mag) |
- |
H (mag) |
6.01Ref |
Outbursts |
YesRef |
GALEX NUV (mag) |
- |
K (mag) |
5.51Ref |
Outburst type |
Z AndRef |
IUE |
NoRef |
WISE W1 (mag) |
5.10Ref |
Jets |
- |
FUSE |
NoRef |
WISE W2 (mag) |
5.06Ref |
Resolved nebula |
- |
U (mag) |
- |
WISE W3 (mag) |
5.11Ref |
IPmax (eV) |
54.4Ref |
B (mag) |
15.57Ref |
WISE W4 (mag) |
4.65Ref |
[O III] lines |
YesRef |
V (mag) |
13.85Ref |
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) |
13.33Ref |
IRAS 100μm (Jy) |
- |
|
|
G (mag) |
11.27Ref |
AKARI S09 (Jy) |
- |
|
|
RP (mag) |
9.89Ref |
AKARI S18 (Jy) |
- |
|
|
Orbit
Orbital period (days) |
617.2±7.4Ref, 794±61Ref |
γ velocity (km/h) |
-58.79±0.22Ref |
Size of giant’s orbit (AU) |
0.399Ref |
Eccentricity |
0Ref |
RV of giant (km/h) |
6.47±0.29Ref |
Separation (AU) |
- |
Inclination (°) |
- |
Inferior conj. of giant (JD) |
2451801.1 |
Mass function |
0.0189Ref |
Eclipses |
- |
|
|
Mass ratio |
- |
Orbital ephemeris |
- |
|
|
|
|
Cool component
Spectral type |
M1 IIIRef, M2 IIIRef, M4.3 IIIRef, M5.5 IIIRef |
Mass (M⊙) |
1.5Ref |
Pulsation |
- |
Eff. temperature (K) |
3720Ref, 3300Ref |
Radius (R⊙) |
119-171Ref |
Type |
- |
IR type |
SRef |
Luminosity (L⊙) |
- |
Pulsation period (days) |
- |
Metallicity [Fe/H] |
0.03±0.07Ref |
|
|
Pulsation ephemeris |
- |
Hot component
Type/Spectral type |
- |
Mass (M⊙) |
- |
Spin period (min) |
- |
Shell-burning/Accreting-only |
shell-burningRef |
Radius (R⊙) |
0.013-0.026Ref |
Accretion disk |
- |
Eff. temperature (K) |
124000-145000Ref |
Luminosity (L⊙) |
60-140Ref |
|
|
Lower limit (K) |
- |
|
|
|
|
Upper limit (K) |
- |
|
|
|
|
Notes
The spectrum reported in Merrill & Burwell (1950) displayed very strong Balmer lines along with TiO bands. In Allen (1978), the detection of He I, [O III], and He II is noted.
References
- Allen, D. A., 1978, MNRAS, 184, 601, 1978MNRAS.184..601A
- Fekel, F. C., Hinkle, K. H., Joyce, R. R. et al., 2007, AJ, 133, 1, 17, 2007AJ....133...17F
- Gromadzki, M., Mikołajewska, J., Soszyński, I., 2013, AcA, 63, 4, 405, 2013AcA....63..405G
- Gutiérrez-Moreno, A., Moreno, H., Costa, E., 1999, PASP, 111, 759, 571, 1999PASP..111..571G
- Medina Tanco, G. A., Steiner, J. E., 1995, AJ, 109, 1770, 1995AJ....109.1770M
- Merrill, P. W., Burwell, C. G., 1950, ApJ, 112, 72, 1950ApJ...112...72M
- Mürset, U., Schmid, H. M., 1999, A&AS, 137, 473, 1999A&AS..137..473M
- Sanduleak, N., Stephenson, C. B., 1973, ApJ, 185, 899, 1973ApJ...185..899S
Last updated: April 18, 2022