NSV 22840
CONFIRMED
MILKY WAY
Constellation
Ophiucus |
Equatorial coordinates
α = 17 35 58.474
δ = -28 49 54.228 |
Galactic coordinates
l = 358.9699°
b = 1.8460° |
Suspected |
2013Ref |
Confirmed |
2013Ref |
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) |
NSV 22840 (Conf.) |
Boyarchuk (1969) |
- |
Vaidis (1988, 1991) |
- |
Position
Right ascension (°) |
263.9936Ref |
Parallax (mas) |
0.004±0.076Ref |
Reddening E(B-V) (mag) |
1.64±0.12Ref, Note |
Declination (°) |
-28.8317Ref |
Distance (kpc) |
8.52Ref, Note, 5.62Ref, Note |
|
|
Galactic longitude (°) |
358.9699Ref |
Proper motion in α (mas/yr) |
4.45±0.09Ref |
|
|
Galactic latitude (°) |
1.8460Ref |
Proper motion in δ (mas/yr) |
-5.47±0.06Ref |
|
|
Observations
X-Ray |
NoRef |
IR type |
SRef |
Radio |
- |
X-Ray type |
- |
J (mag) |
10.50Ref |
Flickering |
- |
GALEX FUV (mag) |
- |
H (mag) |
9.20Ref |
Outbursts |
- |
GALEX NUV (mag) |
- |
K (mag) |
8.65Ref |
Outburst type |
- |
IUE |
NoRef |
WISE W1 (mag) |
8.21Ref |
Jets |
- |
FUSE |
NoRef |
WISE W2 (mag) |
8.19Ref |
Resolved nebula |
- |
U (mag) |
- |
WISE W3 (mag) |
7.63Ref |
IPmax (eV) |
54.4Ref |
B (mag) |
- |
WISE W4 (mag) |
7.10Ref |
[O III] lines |
YesRef |
V (mag) |
17.70Ref |
IRAS 12μm (Jy) |
- |
He II lines |
YesRef |
R (mag) |
15.80Ref |
IRAS 25μm (Jy) |
- |
[Fe VII] lines |
NoRef |
I (mag) |
- |
IRAS 60μm (Jy) |
- |
O VI lines |
NoRef |
BP (mag) |
17.36Ref |
IRAS 100μm (Jy) |
- |
|
|
G (mag) |
15.01Ref |
AKARI S09 (Jy) |
- |
|
|
RP (mag) |
13.55Ref |
AKARI S18 (Jy) |
- |
|
|
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 |
Yes?Ref |
|
|
Mass ratio |
- |
Orbital ephemeris |
- |
|
|
|
|
Cool component
Spectral type |
M0-3Ref |
Mass (M⊙) |
- |
Pulsation |
YesRef |
Eff. temperature (K) |
- |
Radius (R⊙) |
- |
Type |
SRRef |
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) |
55000Ref |
|
|
|
|
Upper limit (K) |
- |
|
|
|
|
Notes
The spectrum of this star confirms its S-type symbiotic nature, and the OGLE-IV light curve reveals potential eclipse in addition to semi-regular pulsations, as detailed in Miszalski et al. (2013).
References
- Miszalski, B., Mikołajewska, J., Udalski, A., 2013, MNRAS, 432, 4, 3186, 2013MNRAS.432.3186M
Last updated: November 5, 2019