Terz V 2513
CONFIRMED
MILKY WAY
Constellation
Ophiucus |
Equatorial coordinates
α = 17 33 47.261
δ = -27 19 26.425 |
Galactic coordinates
l = 359.9792°
b = 3.0664° |
| Suspected |
2014Ref |
| Confirmed |
2014Ref |
| Symbiotic IR type |
SRef |
| Hot component type |
shell-burningRef |
| Outbursts |
YesRef - SyN or Z AndRef |
|
|
Symbiotic Catalogs
| Bidelman (1954) |
- |
Allen (1984) |
- |
Belzcyński et al. (2001) |
- |
| Gaposchkin (1957) |
- |
Kenyon (1986) |
- |
Akras et al. (2019) |
2MASSJ17334728-2719266 (Conf.) |
| Boyarchuk (1969) |
- |
Vaidis (1988, 1991) |
- |
Position
| Right ascension (°) |
263.4469Ref |
Parallax (mas) |
-0.287±0.129Ref |
Reddening E(B-V) (mag) |
1.58±0.05Ref, Note |
| Declination (°) |
-27.3240Ref |
Distance (kpc) |
9.27Ref, Note, 6.70Ref, Note |
|
|
| Galactic longitude (°) |
359.9792Ref |
Proper motion in α (mas/yr) |
-2.10±0.16Ref |
|
|
| Galactic latitude (°) |
3.0664Ref |
Proper motion in δ (mas/yr) |
-10.03±0.11Ref |
|
|
Observations
| X-Ray |
NoRef |
IR type |
SRef |
Radio |
- |
| X-Ray type |
- |
J (mag) |
9.32Ref |
Flickering |
- |
| GALEX FUV (mag) |
- |
H (mag) |
7.91Ref |
Outbursts |
YesRef |
| GALEX NUV (mag) |
- |
K (mag) |
7.26Ref |
Outburst type |
SyN or Z AndRef |
| IUE |
NoRef |
WISE W1 (mag) |
6.32Ref |
Jets |
- |
| FUSE |
NoRef |
WISE W2 (mag) |
5.87Ref |
Resolved nebula |
- |
| U (mag) |
- |
WISE W3 (mag) |
4.73Ref |
IPmax (eV) |
54.4Ref |
| B (mag) |
- |
WISE W4 (mag) |
4.03Ref |
[O III] lines |
YesRef |
| V (mag) |
- |
IRAS 12μm (Jy) |
- |
He II lines |
YesRef |
| R (mag) |
- |
IRAS 25μm (Jy) |
- |
[Fe VII] lines |
NoRef |
| I (mag) |
- |
IRAS 60μm (Jy) |
- |
O VI lines |
NoRef |
| BP (mag) |
16.59Ref |
IRAS 100μm (Jy) |
- |
|
|
| G (mag) |
14.85Ref |
AKARI S09 (Jy) |
0.54Ref |
|
|
| RP (mag) |
12.51Ref |
AKARI S18 (Jy) |
0.33Ref |
|
|
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 |
M2Ref |
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
An increase of up to 5.0 magnitudes was observed, that could be attributed to either a Z And outburst or a symbiotic nova outburst, as discussed in Miszalski & Mikołajewska (2014).
Last updated: May 11, 2021