LAMOST J043858.27+263108.4
SUSPECTED
MILKY WAY
Constellation
Taurus |
Equatorial coordinates
α = 04 38 58.281
δ = +26 31 08.559 |
Galactic coordinates
l = 173.3183°
b = -13.3846° |
| Suspected |
2023Ref |
| Confirmed |
- |
| Symbiotic IR type |
- |
| Hot component type |
accreting-onlyRef |
| 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 (°) |
69.7428Ref |
Parallax (mas) |
0.009±0.088Ref |
Reddening E(B-V) (mag) |
1.63±0.05Ref, Note |
| Declination (°) |
26.5190Ref |
Distance (kpc) |
4.47Ref, Note
-, Note |
|
|
| Galactic longitude (°) |
173.3183Ref |
Proper motion in α (mas/yr) |
0.65±0.12Ref |
|
|
| Galactic latitude (°) |
-13.3846Ref |
Proper motion in δ (mas/yr) |
-0.68±0.08Ref |
|
|
Observations
| X-Ray |
- |
IR type |
- |
Radio |
- |
| X-Ray type |
- |
J (mag) |
9.42Ref |
Flickering |
- |
| GALEX FUV (mag) |
- |
H (mag) |
7.69Ref |
Outbursts |
- |
| GALEX NUV (mag) |
- |
K (mag) |
6.89Ref |
Outburst type |
- |
| IUE |
NoRef |
WISE W1 (mag) |
6.43Ref |
Jets |
- |
| FUSE |
NoRef |
WISE W2 (mag) |
6.26Ref |
Resolved nebula |
- |
| U (mag) |
- |
WISE W3 (mag) |
5.45Ref |
IPmax (eV) |
- |
| B (mag) |
- |
WISE W4 (mag) |
4.50Ref |
[O III] lines |
- |
| V (mag) |
- |
IRAS 12μm (Jy) |
- |
He II lines |
- |
| R (mag) |
15.60Ref |
IRAS 25μm (Jy) |
- |
[Fe VII] lines |
- |
| I (mag) |
- |
IRAS 60μm (Jy) |
- |
O VI lines |
- |
| BP (mag) |
19.06Ref |
IRAS 100μm (Jy) |
- |
|
|
| G (mag) |
14.81Ref |
AKARI S09 (Jy) |
0.28Ref |
|
|
| RP (mag) |
13.22Ref |
AKARI S18 (Jy) |
0.23Ref |
|
|
Orbit
| Orbital period (days) |
- |
γ velocity (km/h) |
-39.25±2.44Ref |
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 |
M5Ref |
Mass (M⊙) |
- |
Pulsation |
- |
| Eff. temperature (K) |
- |
Radius (R⊙) |
- |
Type |
- |
| IR type |
- |
Luminosity (L⊙) |
- |
Pulsation period (days) |
- |
| Metallicity [Fe/H] |
- |
|
|
Pulsation ephemeris |
- |
Hot component
| Type/Spectral type |
- |
Mass (M⊙) |
- |
Spin period (min) |
- |
| Shell-burning/Accreting-only |
accreting-onlyRef |
Radius (R⊙) |
- |
Accretion disk |
- |
| Eff. temperature (K) |
- |
Luminosity (L⊙) |
- |
|
|
| Lower limit (K) |
- |
|
|
|
|
| Upper limit (K) |
- |
|
|
|
|
Notes
Suspected of having a symbiotic nature by Jia et al. (2023) based on the machine-learning search. The spectra from the SDSS survey suggest an accreting-only nature.
References
- Jia, Y., Guo, S., Zhu, C. et al., 2023, RAA, 23, 10, 105012, 2023RAA....23j5012J
Last updated: January 13, 2024