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