Gaia DR3 4174300945736308480
SUSPECTED
MILKY WAY
Constellation
Serpens |
Equatorial coordinates
α = 18 11 24.175
δ = -04 25 06.886 |
Galactic coordinates
l = 24.3839°
b = 6.8395° |
| Suspected |
2022Ref |
| Confirmed |
- |
| Symbiotic IR type |
- |
| Hot component type |
- |
| 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 (°) |
272.8507Ref |
Parallax (mas) |
0.019±0.035Ref |
Reddening E(B-V) (mag) |
1.1±0.03Ref, Note |
| Declination (°) |
-4.4186Ref |
Distance (kpc) |
8.58Ref, Note, 7.50Ref, Note |
|
|
| Galactic longitude (°) |
24.3839Ref |
Proper motion in α (mas/yr) |
-4.24±0.03Ref |
|
|
| Galactic latitude (°) |
6.8395Ref |
Proper motion in δ (mas/yr) |
-3.69±0.03Ref |
|
|
Observations
| X-Ray |
- |
IR type |
- |
Radio |
- |
| X-Ray type |
- |
J (mag) |
11.06Ref |
Flickering |
- |
| GALEX FUV (mag) |
- |
H (mag) |
9.93Ref |
Outbursts |
- |
| GALEX NUV (mag) |
- |
K (mag) |
9.53Ref |
Outburst type |
- |
| IUE |
NoRef |
WISE W1 (mag) |
9.35Ref |
Jets |
- |
| FUSE |
NoRef |
WISE W2 (mag) |
9.36Ref |
Resolved nebula |
- |
| U (mag) |
- |
WISE W3 (mag) |
9.10Ref |
IPmax (eV) |
- |
| B (mag) |
- |
WISE W4 (mag) |
8.34Ref |
[O III] lines |
- |
| V (mag) |
- |
IRAS 12μm (Jy) |
- |
He II lines |
- |
| R (mag) |
- |
IRAS 25μm (Jy) |
- |
[Fe VII] lines |
- |
| I (mag) |
- |
IRAS 60μm (Jy) |
- |
O VI lines |
- |
| BP (mag) |
16.69Ref |
IRAS 100μm (Jy) |
- |
|
|
| G (mag) |
14.69Ref |
AKARI S09 (Jy) |
- |
|
|
| RP (mag) |
13.38Ref |
AKARI S18 (Jy) |
- |
|
|
Orbit
| Orbital period (days) |
- |
γ velocity (km/h) |
-110.39±2.23Ref |
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 |
M?Ref |
Mass (M⊙) |
- |
Pulsation |
Yes?Ref |
| Eff. temperature (K) |
- |
Radius (R⊙) |
- |
Type |
SRRef |
| IR type |
- |
Luminosity (L⊙) |
- |
Pulsation period (days) |
409Ref |
| Metallicity [Fe/H] |
- |
|
|
Pulsation ephemeris |
- |
Hot component
| Type/Spectral type |
- |
Mass (M⊙) |
- |
Spin period (min) |
- |
| Shell-burning/Accreting-only |
- |
Radius (R⊙) |
- |
Accretion disk |
- |
| Eff. temperature (K) |
- |
Luminosity (L⊙) |
- |
|
|
| Lower limit (K) |
- |
|
|
|
|
| Upper limit (K) |
- |
|
|
|
|
Notes
Classified as a symbiotic star by Rimoldini et al. (2023) based on a machine-learning technique applied to Gaia DR3 data, including astrometric, photometric, and photometric time series information. Periodicity of 409 days was reported by Jayasinghe et al. (2018).
References
- Jayasinghe, T., Kochanek, C. S., Stanek, K. Z. et al., 2018, MNRAS, 477, 3, 3145, 2018MNRAS.477.3145J
- Rimoldini, L., Holl, B., Gavras, P. et al., 2023, A&A, 674, A14, 2023A&A...674A..14R
Last updated: January 16, 2023