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