[KW2003] 95
CONFIRMED
MILKY WAY
Constellation
Sagittarius |
Equatorial coordinates
α = 18 11 23.208
δ = -24 14 30.091 |
Galactic coordinates
l = 6.9445°
b = -2.6437° |
| Suspected |
2019Ref |
| Confirmed |
2021Ref |
| Symbiotic IR type |
SRef |
| Hot component type |
shell-burningRef |
| Outbursts |
- |
|
|
Symbiotic Catalogs
| Bidelman (1954) |
- |
Allen (1984) |
- |
Belzcyński et al. (2001) |
- |
| Gaposchkin (1957) |
- |
Kenyon (1986) |
- |
Akras et al. (2019) |
- |
| Boyarchuk (1969) |
- |
Vaidis (1988, 1991) |
- |
Position
| Right ascension (°) |
272.8467Ref |
Parallax (mas) |
0.101±0.031Ref |
Reddening E(B-V) (mag) |
1.36±0.12Ref, Note |
| Declination (°) |
-24.2417Ref |
Distance (kpc) |
6.13Ref, Note, 5.62Ref, Note |
|
|
| Galactic longitude (°) |
6.9445Ref |
Proper motion in α (mas/yr) |
-3.62±0.04Ref |
|
|
| Galactic latitude (°) |
-2.6437Ref |
Proper motion in δ (mas/yr) |
-11.10±0.03Ref |
|
|
Observations
| X-Ray |
NoRef |
IR type |
SRef |
Radio |
- |
| X-Ray type |
- |
J (mag) |
11.13Ref |
Flickering |
- |
| GALEX FUV (mag) |
- |
H (mag) |
9.86Ref |
Outbursts |
- |
| GALEX NUV (mag) |
- |
K (mag) |
9.37Ref |
Outburst type |
- |
| IUE |
NoRef |
WISE W1 (mag) |
8.87Ref |
Jets |
- |
| FUSE |
NoRef |
WISE W2 (mag) |
8.84Ref |
Resolved nebula |
- |
| U (mag) |
- |
WISE W3 (mag) |
8.46Ref |
IPmax (eV) |
54.4Ref |
| B (mag) |
- |
WISE W4 (mag) |
7.61Ref |
[O III] lines |
YesRef |
| V (mag) |
16.60Ref |
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) |
16.80Ref |
IRAS 100μm (Jy) |
- |
|
|
| G (mag) |
14.98Ref |
AKARI S09 (Jy) |
- |
|
|
| RP (mag) |
13.70Ref |
AKARI S18 (Jy) |
- |
|
|
Orbit
| Orbital period (days) |
- |
γ velocity (km/h) |
- |
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 |
- |
|
|
|
|
Cool component
| Spectral type |
KRef |
Mass (M⊙) |
- |
Pulsation |
- |
| Eff. temperature (K) |
- |
Radius (R⊙) |
- |
Type |
- |
| IR type |
SRef |
Luminosity (L⊙) |
- |
Pulsation period (days) |
- |
| Metallicity [Fe/H] |
- |
|
|
Pulsation ephemeris |
- |
Hot component
| Type/Spectral type |
- |
Mass (M⊙) |
- |
Spin period (min) |
- |
| Shell-burning/Accreting-only |
shell-burningRef |
Radius (R⊙) |
- |
Accretion disk |
- |
| Eff. temperature (K) |
- |
Luminosity (L⊙) |
- |
|
|
| Lower limit (K) |
- |
|
|
|
|
| Upper limit (K) |
- |
|
|
|
|
Notes
Previously classified as a possible symbiotic star by Akras et al. (2019) based on a machine learning approach. Spectroscopic observations presented by Akras et al. (2021) confirmed the symbiotic nature.
References
- Akras, S., Gonçalves, D. R., Alvarez-Candal, A. et al., 2021, MNRAS, 502, 2, 2513, 2021MNRAS.502.2513A
- Akras, S., Leal-Ferreira, M. L., Guzman-Ramirez, L. et al., 2019, MNRAS, 483, 4, 5077, 2019MNRAS.483.5077A
Last updated: April 12, 2021