NSV 20400
CONFIRMED
MILKY WAY
Constellation
Lupus |
Equatorial coordinates
α = 15 47 50.755
δ = -32 43 59.364 |
Galactic coordinates
l = 340.6598°
b = 16.9207° |
| Suspected |
2020Ref |
| 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 (°) |
236.9615Ref |
Parallax (mas) |
0.119±0.042Ref |
Reddening E(B-V) (mag) |
0.12±0.0Ref, Note |
| Declination (°) |
-32.7332Ref |
Distance (kpc) |
6.90Ref, Note, 6.14Ref, Note |
|
|
| Galactic longitude (°) |
340.6598Ref |
Proper motion in α (mas/yr) |
-9.68±0.05Ref |
|
|
| Galactic latitude (°) |
16.9207Ref |
Proper motion in δ (mas/yr) |
0.17±0.04Ref |
|
|
Observations
| X-Ray |
- |
IR type |
SRef |
Radio |
- |
| X-Ray type |
- |
J (mag) |
8.40Ref |
Flickering |
YesRef |
| GALEX FUV (mag) |
- |
H (mag) |
7.50Ref |
Outbursts |
- |
| GALEX NUV (mag) |
- |
K (mag) |
7.12Ref |
Outburst type |
- |
| IUE |
NoRef |
WISE W1 (mag) |
6.90Ref |
Jets |
- |
| FUSE |
NoRef |
WISE W2 (mag) |
7.07Ref |
Resolved nebula |
- |
| U (mag) |
- |
WISE W3 (mag) |
6.71Ref |
IPmax (eV) |
54.4Ref |
| B (mag) |
14.15Ref |
WISE W4 (mag) |
6.53Ref |
[O III] lines |
YesRef |
| V (mag) |
12.90Ref |
IRAS 12μm (Jy) |
- |
He II lines |
YesRef |
| R (mag) |
13.43Ref |
IRAS 25μm (Jy) |
- |
[Fe VII] lines |
NoRef |
| I (mag) |
10.28Ref |
IRAS 60μm (Jy) |
- |
O VI lines |
NoRef |
| BP (mag) |
13.93Ref |
IRAS 100μm (Jy) |
- |
|
|
| G (mag) |
11.99Ref |
AKARI S09 (Jy) |
0.15Ref |
|
|
| RP (mag) |
10.57Ref |
AKARI S18 (Jy) |
- |
|
|
Orbit
| Orbital period (days) |
895Ref |
γ velocity (km/h) |
-95.47±1.33Ref |
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 |
SRef |
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
Symbiotic candidate selected for AAVSO observing campaing (Waagen, 2020) by Adrian B. Lucy (Columbia University). Subsequently confirmed as a symbiotic star by Lucy (2021).
References
- Bidelman, W. P., 1991, IBVS, 3617, 1, 1991IBVS.3617....1B
- Lucy, A. B., 2021, PhDT, 1, 2021PhDT........17L
- Merc, J., Beck, P. G., Mathur, S. et al., 2023, arXiv, arXiv:2312.16126, 2023arXiv231216126M
- Waagen, E. O., 2020, AAVSO Alert Notice, 708, 1, 2020AAN...708....1W
Last updated: January 12, 2024