ASASSN-V J081823.00-111138.9
SUSPECTED
MILKY WAY
Constellation
Hydra |
Equatorial coordinates
α = 08 18 23.001
δ = -11 11 38.928 |
Galactic coordinates
l = 233.3071°
b = 13.5800° |
| Suspected |
2018Ref |
| Confirmed |
- |
| Symbiotic IR type |
S?Ref |
| Hot component type |
accreting-only?Ref |
| 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 (°) |
124.5958Ref |
Parallax (mas) |
0.226±0.022Ref |
Reddening E(B-V) (mag) |
0.08±0.01Ref, Note |
| Declination (°) |
-11.1941Ref |
Distance (kpc) |
4.12Ref, Note, 3.82Ref, Note |
|
|
| Galactic longitude (°) |
233.3071Ref |
Proper motion in α (mas/yr) |
-0.61±0.02Ref |
|
|
| Galactic latitude (°) |
13.5800Ref |
Proper motion in δ (mas/yr) |
1.21±0.02Ref |
|
|
Observations
| X-Ray |
- |
IR type |
S?Ref |
Radio |
- |
| X-Ray type |
- |
J (mag) |
8.74Ref |
Flickering |
- |
| GALEX FUV (mag) |
- |
H (mag) |
7.84Ref |
Outbursts |
- |
| GALEX NUV (mag) |
- |
K (mag) |
7.50Ref |
Outburst type |
- |
| IUE |
NoRef |
WISE W1 (mag) |
7.28Ref |
Jets |
- |
| FUSE |
NoRef |
WISE W2 (mag) |
7.24Ref |
Resolved nebula |
- |
| U (mag) |
- |
WISE W3 (mag) |
5.58Ref |
IPmax (eV) |
- |
| B (mag) |
14.34Ref |
WISE W4 (mag) |
4.54Ref |
[O III] lines |
- |
| V (mag) |
12.50Ref |
IRAS 12μm (Jy) |
0.20Ref |
He II lines |
- |
| R (mag) |
11.99Ref |
IRAS 25μm (Jy) |
0.11Ref |
[Fe VII] lines |
- |
| I (mag) |
10.18Ref |
IRAS 60μm (Jy) |
0.19Ref |
O VI lines |
- |
| BP (mag) |
12.86Ref |
IRAS 100μm (Jy) |
1.06Ref |
|
|
| G (mag) |
11.53Ref |
AKARI S09 (Jy) |
0.22Ref |
|
|
| RP (mag) |
10.39Ref |
AKARI S18 (Jy) |
- |
|
|
Orbit
| Orbital period (days) |
- |
γ velocity (km/h) |
104.11±0.43Ref |
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 |
- |
Mass (M⊙) |
- |
Pulsation |
- |
| Eff. temperature (K) |
- |
Radius (R⊙) |
- |
Type |
- |
| IR type |
S?Ref |
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-only?Ref |
Radius (R⊙) |
- |
Accretion disk |
- |
| Eff. temperature (K) |
- |
Luminosity (L⊙) |
- |
|
|
| Lower limit (K) |
- |
|
|
|
|
| Upper limit (K) |
- |
|
|
|
|
Notes
Symbiotic candidate selected for AAVSO observing campaing (AAVSO Alert Notice 632) by Adrian B. Lucy (Columbia University).
References
- Angeloni, R., Gonçalves, D. R., Akras, S. et al., 2019, AJ, 157, 4, 156, 2019AJ....157..156A
- Buder, S., Asplund, M., Duong, L. et al., 2018, MNRAS, 478, 4, 4513, 2018MNRAS.478.4513B
Last updated: August 23, 2021