ER Oph
SUSPECTED
MILKY WAY
Constellation
Ophiucus |
Equatorial coordinates
α = 17 00 42.128
δ = -26 10 12.688 |
Galactic coordinates
l = 356.6858°
b = 9.7872° |
Suspected |
2018Ref |
Confirmed |
- |
Symbiotic IR type |
S?Ref |
Hot component type |
accreting-only?Ref |
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 (°) |
255.1755Ref |
Parallax (mas) |
0.341±0.051Ref |
Reddening E(B-V) (mag) |
0.25±0.01Ref, Note |
Declination (°) |
-26.1702Ref |
Distance (kpc) |
2.96Ref, Note, 3.66Ref, Note |
|
|
Galactic longitude (°) |
356.6858Ref |
Proper motion in α (mas/yr) |
-4.85±0.07Ref |
|
|
Galactic latitude (°) |
9.7872Ref |
Proper motion in δ (mas/yr) |
-5.78±0.05Ref |
|
|
Observations
X-Ray |
- |
IR type |
S?Ref |
Radio |
- |
X-Ray type |
- |
J (mag) |
8.49Ref |
Flickering |
- |
GALEX FUV (mag) |
- |
H (mag) |
7.67Ref |
Outbursts |
- |
GALEX NUV (mag) |
- |
K (mag) |
7.25Ref |
Outburst type |
- |
IUE |
NoRef |
WISE W1 (mag) |
6.85Ref |
Jets |
- |
FUSE |
NoRef |
WISE W2 (mag) |
6.44Ref |
Resolved nebula |
- |
U (mag) |
- |
WISE W3 (mag) |
5.61Ref |
IPmax (eV) |
- |
B (mag) |
16.43Ref |
WISE W4 (mag) |
4.78Ref |
[O III] lines |
- |
V (mag) |
11.80Ref |
IRAS 12μm (Jy) |
- |
He II lines |
- |
R (mag) |
- |
IRAS 25μm (Jy) |
- |
[Fe VII] lines |
- |
I (mag) |
- |
IRAS 60μm (Jy) |
- |
O VI lines |
- |
BP (mag) |
15.47Ref |
IRAS 100μm (Jy) |
- |
|
|
G (mag) |
12.67Ref |
AKARI S09 (Jy) |
0.28Ref |
|
|
RP (mag) |
11.06Ref |
AKARI S18 (Jy) |
- |
|
|
Orbit
Orbital period (days) |
- |
γ velocity (km/h) |
-130.64±1.47Ref |
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 |
YesRef |
Eff. temperature (K) |
- |
Radius (R⊙) |
- |
Type |
MiraRef |
IR type |
S?Ref |
Luminosity (L⊙) |
- |
Pulsation period (days) |
208.76±1.83Ref |
Metallicity [Fe/H] |
- |
|
|
Pulsation ephemeris |
- |
Hot component
Type/Spectral type |
- |
Mass (M⊙) |
- |
Spin period (min) |
- |
Shell-burning/Accreting-only |
accreting-only?Ref |
Radius (R⊙) |
- |
Accretion disk |
- |
Eff. temperature (K) |
- |
Luminosity (L⊙) |
- |
|
|
Lower limit (K) |
- |
|
|
|
|
Upper limit (K) |
- |
|
|
|
|
Notes
Symbiotic candidate selected for AAVSO observing campaing (AAVSO Alert Notice 650) by Adrian B. Lucy (Columbia University). Classified as a Mira variable by Pojmanski (2002).
References
- Pojmanski, G., 2002, AcA, 52, 397, 2002AcA....52..397P
- Vogt, N., Contreras-Quijada, A., Fuentes-Morales, I. et al., 2016, ApJS, 227, 1, 6, 2016ApJS..227....6V
Last updated: August 23, 2021