2MASS J16422739-4133105
CONFIRMED
MILKY WAY
Constellation
Scorpius |
Equatorial coordinates
α = 16 42 27.385
δ = -41 33 10.630 |
Galactic coordinates
l = 342.2640°
b = 3.0318° |
Suspected |
2014Ref |
Confirmed |
2014Ref |
Symbiotic IR type |
SRef, DRef |
Hot component type |
shell-burningRef |
Outbursts |
- |
|
|
Symbiotic Catalogs
Bidelman (1954) |
- |
Allen (1984) |
- |
Belzcyński et al. (2001) |
- |
Gaposchkin (1957) |
- |
Kenyon (1986) |
- |
Akras et al. (2019) |
2MASSJ16422739-4133105 (Conf.) |
Boyarchuk (1969) |
- |
Vaidis (1988, 1991) |
- |
Position
Right ascension (°) |
250.6141Ref |
Parallax (mas) |
0.003±0.073Ref |
Reddening E(B-V) (mag) |
1.43±0.09Ref, Note |
Declination (°) |
-41.5530Ref |
Distance (kpc) |
7.87Ref, Note, 7.83Ref, Note |
|
|
Galactic longitude (°) |
342.2640Ref |
Proper motion in α (mas/yr) |
-4.42±0.11Ref |
|
|
Galactic latitude (°) |
3.0318Ref |
Proper motion in δ (mas/yr) |
-3.77±0.09Ref |
|
|
Observations
X-Ray |
- |
IR type |
SRef, DRef |
Radio |
- |
X-Ray type |
- |
J (mag) |
10.33Ref |
Flickering |
- |
GALEX FUV (mag) |
- |
H (mag) |
8.96Ref |
Outbursts |
- |
GALEX NUV (mag) |
- |
K (mag) |
7.66Ref |
Outburst type |
- |
IUE |
NoRef |
WISE W1 (mag) |
6.09Ref |
Jets |
- |
FUSE |
NoRef |
WISE W2 (mag) |
4.94Ref |
Resolved nebula |
- |
U (mag) |
- |
WISE W3 (mag) |
3.99Ref |
IPmax (eV) |
114Ref |
B (mag) |
- |
WISE W4 (mag) |
3.30Ref |
[O III] lines |
YesRef |
V (mag) |
- |
IRAS 12μm (Jy) |
1.69Ref |
He II lines |
YesRef |
R (mag) |
- |
IRAS 25μm (Jy) |
0.76Ref |
[Fe VII] lines |
YesRef |
I (mag) |
- |
IRAS 60μm (Jy) |
3.85Ref |
O VI lines |
YesRef |
BP (mag) |
17.13Ref |
IRAS 100μm (Jy) |
30.40Ref |
|
|
G (mag) |
16.40Ref |
AKARI S09 (Jy) |
0.95Ref |
|
|
RP (mag) |
15.35Ref |
AKARI S18 (Jy) |
0.57Ref |
|
|
Orbit
Orbital period (days) |
- |
γ velocity (km/h) |
- |
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 |
SRef, DRef |
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
The red giant in this system has not been detected, likely obscured by dust and therefore not visible at optical wavelengths, as indicated by Miszalski & Mikołajewska (2014).
Last updated: November 20, 2019